A Cellular Scale Study of Low Density Lipoprotein Concentration Polarisation in Arteries
by
P. E. Vincent
Department of Aeronautics Imperial College London Prince Consort Road London SW7 2BY
This thesis is submitted for the degree of Doctor of Philosophy of the University of London
2009 Declaration
This is to certify that the work presented in this thesis has been carried out at Imperial College London and has not been previously submitted to any other university or technical institution for a degree or award. I further certify that all material in this thesis which is not my own work has been properly acknowledged.
P. E. Vincent Abstract
Uptake of Low Density Lipoprotein (LDL) by the arterial wall is likely to play a key role in the process of atherogenesis, which occurs non-uniformly within the ar- terial vasculature. A particular process that may cause vascular scale heterogeneity in the rate of transendothelial LDL transport is the formation of a flow-dependent LDL concentration polarisation layer adjacent to the luminal surface of the arte- rial endothelium. In this thesis the effects of cellular scale endothelial features on such LDL concentration polarisation are investigated using an idealised theoretical model. Specifically, the effect of a spatially heterogeneous transmural water flux is considered (flowing only through intercellular clefts), as well as the effect of the endothelial glycocalyx layer (EGL). The idealised model is implemented using both analytical techniques and the spectral/hp element method. A range of scenarios are considered, including those were no EGL is present, those where an EGL is present but LDL cannot penetrate into it, and finally those where an EGL is present and LDL can penetrate into it.
For cases where no EGL is present, particular attention is paid to the spatially averaged LDL concentration adjacent to various regions of the endothelial surface, as such measures may be relevant to the rate of transendothelial LDL transport. It is demonstrated, in principle, that a heterogeneous transmural water flux alone can act to enhance such measures, and cause them to develop a shear dependence (in addition to that caused by vascular scale flow features affecting the overall degree of LDL concentration polarisation). However, it is shown that this enhancement and additional shear dependence are likely to be negligible for a physiologically realistic transmural flux velocity of 0.0439µms−1 and an LDL diffusivity in blood plasma of 28.67µm2s−1.
For cases where an EGL is present, measures of LDL concentration polarisation relevant to the rate of transendothelial LDL transport can also be defined. It is demonstrated that an EGL is unlikely to cause any additional shear dependence of such measures directly, irrespective of whether or not LDL can penetrate into the EGL. However, it is found that such measures depend significantly on the nature of the interaction between LDL and the EGL (parameterised by the height of the EGL, the depth to which LDL penetrates into the EGL, and the diffusivity of LDL within the EGL). Various processes may regulate the interaction of LDL with the EGL, possibly in a flow dependent and hence spatially non-uniform fashion. It is concluded that any such processes may be as important as vascular scale flow features in terms of spatially modulating transendothelial LDL transport via an LDL concentration polarisation mechanism.
3 Acknowledgments
I would like to begin by thanking Prof. Colin Caro and Prof. Spencer Sherwin for giving me the opportunity to do my PhD in such a diverse and interesting field of research. I would like to thank Prof. Spencer Sherwin and Prof. Peter Weinberg for their excellent supervision. I would like to thank Prof. Kim Parker, Prof. Charles Michel, Prof. John Tarbell, Prof. Sheldon Weinbaum, Prof. David Rumschitzki, Prof. Darren Crowdy, Prof. Aaron Fogelson and Dr. Leopold Grinberg for their wisdom and assistance. I would like to thank all of my office mates, especially Donal and Andy, for all the useful discussions. I would like to thank Hakan and Marcus for all of their sensible thoughts. Finally, I would like to thank Ana for all of her love and support (especially the besitos and paella), and my parents for their unwavering support and understanding throughout the last 25 years.
This work was funded by the Engineering and Physical Sciences Research Council (UK). Nomenclature
b∗ Distance LDL can penetrate into the EGL b Non-dimensional distance LDL can penetrate into the EGL ∗ C Profile of generic macroscale LDL concentration polarisation layer
∗ CB LDL concentration in bulk blood flow ∗ CE LDL concentration adjacent to luminal surface of endothelium ∗ CW LDL concentration within arterial wall ∗ Cα LDL concentration field within ΩαC
Cα Non-dimensional LDL concentration field within ΩαC ∗ Cα Profile of macroscale LDL concentration polarisation layer when no EGL is considered
Cα Non-dimensional profile of macroscale LDL concentration polarisation layer when no EGL is considered
CαN Spatially averaged non-dimensional LDL concentration to which the endothelium is exposed (in vicinity of cleft entrances when no EGL is considered)
∗ Cαt Time dependent LDL concentration field within ΩαC
Cαt Non-dimensional time dependent LDL concentration field within ΩαC
CαtN Temporally and spatially averaged non-dimensional LDL concentration to which the endothelium is exposed (in vicinity of cleft entrances when no EGL is considered)
CαtU Temporally and spatially averaged non-dimensional LDL concentration to which the endothelium is exposed (when no EGL is considered) CαU Spatially averaged non-dimensional LDL concentration to which the endothelium is exposed (when no EGL is considered)
∗ Cβ LDL concentration field within ΩβC
Cβ Non-dimensional LDL concentration field within ΩβC ∗ Cβ Profile of macroscale LDL concentration polarisation layer when EGL is considered
Cβ Non-dimensional profile of macroscale LDL concentration polarisation layer when EGL is considered
CβN Spatially averaged non-dimensional LDL concentration to which the endothelium is exposed (in vicinity of cleft entrances when EGL is considered)
CβU Spatially averaged non-dimensional LDL concentration to which the endothelium is exposed (when EGL is considered) Da Non-dimensional inverse Darcy permeability tensor within the EGL
∗ DG LDL diffusivity within the EGL ∗ DL LDL diffusivity within the lumen
Dr Ratio of LDL diffusivity in the EGL to LDL diffusivity in the lumen
Dax Inverse of first eigenvalue of Da
Day Inverse of second eigenvalue of Da ∗ ∗ ∗ f Half-distance over which LDL diffusivity varies between DL and DG f Non-dimensional half-distance over which LDL diffusivity varies
∗ ∗ between DL and DG h∗ Height of EGL h Non-dimensional height of EGL
∗ JB LDL flux from bulk flow to endothelial surface ∗ JE LDL flux across endothelium K∗ Inverse Darcy permeability tensor within the EGL
∗ kB Blood side mass transfer coefficient ∗ kE Permeability of endothelium to LDL ∗ ∗ Kx Inverse of first eigenvalue of K
6 ∗ ∗ Ky Inverse of second eigenvalue of K ∗ Lα Height of domain ΩαC
Lα Non-dimensional height of domain ΩαC ∗ Lβ Height of domain ΩβC
Lβ Non-dimensional height of domain ΩβC
P eG Peclet number associated with heterogeneous transmural flux within EGL
P eL Peclet number associated with heterogeneous transmural flux within lumen
∗ pα Pressure field within ΩαV pα Non-dimensional pressure field within ΩαV ∗ pβG Pressure field within ΩβV G pβG Non-dimensional pressure field within ΩβV G ∗ pβL Pressure field within ΩβV L pβL Non-dimensional pressure field within ΩβV L
T Non-dimensional period of γt uα x component of non-dimensional water velocity field vα uαt x component of non-dimensional water velocity field vαt uβG x component of non-dimensional water velocity field vβG uβL x component of non-dimensional water velocity field vβL ∗ V Average transmural water flux velocity vα y component of non-dimensional water velocity field vα ∗ vα Water velocity field within ΩαV vα Non-dimensional water velocity field within ΩαV vαt y component of non-dimensional water velocity field vαt ∗ vαt Time dependent water velocity field within ΩαV vαt Non-dimensional time dependent water velocity field within ΩαV ∗ vβ Water velocity field within ΩβV vβ Non-dimensional water velocity field within ΩβV vβG y component of non-dimensional water velocity field vβG
7 ∗ vβG Water velocity field within ΩβV G vβG Non-dimensional water velocity field within ΩβV G vβL y component of non-dimensional water velocity field vβL ∗ vβL Water velocity field within ΩβV L vβL Non-dimensional water velocity field within ΩβV L γ∗ Shear rate applied orthogonal to length-wise extent of idealised clefts γ Non-dimensional shear rate applied orthogonal to length-wise extent of idealised clefts
∗ ∗ γa Amplitude of γt
γa Non-dimensional amplitude of γt ∗ ∗ γo Offset of γt
γo Non-dimensional offset of γt ∗ γt Time dependent shear rate applied orthogonal to length-wise extent of idealised clefts
γt Non-dimensional time dependent shear rate applied orthogonal to length-wise extent of idealised clefts
∗ γT Shear rate applied to region of interest δ∗ Cleft half-width δ Non-dimensional cleft half-width ∆∗ Cleft half-spacing ζ∗ Thickness of macroscale LDL concentration polarisation layer ζ Non-dimensional thickness of macroscale LDL concentration polarisation layer θ∗ Angle between applied shear and idealised intercellular clefts
κα Non-dimensional distance from endothelium at which Cα becomes approximately one-dimensional
κβ Non-dimensional distance from endothelium at which Cβ becomes approximately one-dimensional µ∗ Dynamic viscosity of water
σα Non-dimensional stress tensor within ΩαV
8 σβG Non-dimensional stress tensor within ΩβV G
σβL Non-dimensional stress tensor within ΩβV L
ψα Stream function within ΩαV
ψβG Stream function within ΩβV G
ψβL Stream function within ΩβV L ∗ ∗ ω Frequency of γt
ω Non-dimensional frequency of γt
ΩαC Domain in which LDL transport is modelled when no EGL is considered
ΩαV Domain in which water motion is modelled when no EGL is considered
ΩβC Domain in which LDL transport is modelled when EGL is considered
ΩβCG Sub-domain of ΩβC that covers EGL
ΩβCL Sub-domain of ΩβC that covers lumen
ΩβV Domain in which water motion is modelled when EGL is considered
ΩβV G Sub-domain of ΩβV that covers EGL
ΩβV L Sub-domain of ΩβV that covers lumen
9 Contents
Declaration 1
Abstract 2
Acknowledgements 4
Nomenclature 5
Table of Contents 10
List of Figures 18
List of Tables 21
1 Introduction 23
1.1 Atherosclerosis ...... 23
1.1.1 Overview ...... 23
1.1.2 Initiation of Atherosclerosis ...... 24
1.1.3 Inter-Human Variation ...... 25
1.1.4 Intra-Human Variation ...... 25 1.2 Blood Flow and Atherosclerosis ...... 26
1.2.1 Overview ...... 26
1.2.2 Regulation by Mechanical Forces ...... 28
1.2.3 Regulation by Mass Transport Mechanisms ...... 28
1.3 Flow Dependent LDL Concentration Polarisation within Arteries . . . 33
1.3.1 Concentration Polarisation ...... 33
1.3.2 LDL Concentration Polarisation within Arteries ...... 34
1.3.3 Flow Dependent LDL Concentration Polarisation within Ar- teries ...... 35
1.3.4 Flow Dependent Regulation of Atherogenesis ...... 37
1.3.5 Previous Studies ...... 37
1.4 Relevant Cellular Scale Features of the Endothelial Surface ...... 38
1.4.1 Spatially Heterogeneous Transmural Water Flux ...... 38
1.4.2 Endothelial Glycocalyx Layer ...... 39
1.5 Objective of Thesis ...... 41
1.6 Overview of Thesis ...... 41
2 Spectral/hp Element Method 42
2.1 Overview ...... 42
2.2 One-Dimensional Spectral/hp Element Method ...... 44
2.2.1 Example Problem ...... 44
2.2.2 Weak Formulation ...... 44
11 2.2.3 An Approximate Solution ...... 45
2.2.4 A Spectral/hp Element Basis ...... 46
2.2.5 Galerkin Approximation ...... 51
2.2.6 Global Matrix Equation ...... 51
2.2.7 Matrix Structure ...... 52
2.2.8 Global Assembly ...... 55
2.2.9 Other Elemental Bases ...... 58
2.3 Extension to Two-Dimensions ...... 58
2.3.1 Overview ...... 58
2.3.2 Basis Functions Within Quadrangular Elements ...... 59
2.3.3 Basis Functions Within Triangular Elements ...... 60
2.4 Advection Diffusion Equation ...... 62
2.4.1 Steady State Two-Dimensional Advection Diffusion Equation . 62
2.4.1.1 Definition ...... 62
2.4.1.2 Weak Form ...... 62
2.4.1.3 Obtaining an Approximate Solution ...... 63
2.4.2 Unsteady Two-Dimensional Advection Diffusion Equation . . 64
2.4.2.1 Definition ...... 64
2.4.2.2 Temporal Discretisation ...... 64
2.4.2.3 Weak Form ...... 65
2.4.2.4 Obtaining an Approximate Solution ...... 66
12 2.5 Summary ...... 67
3 The Effect of a Spatially Heterogeneous Transmural Water Flux 68
3.1 Overview ...... 68
3.2 Idealised Model of Water Flow ...... 69
3.2.1 Heterogeneous Transmural Flux ...... 69
3.2.2 Applied Shear ...... 71
3.2.3 Domain ...... 72
3.2.4 Governing Equations ...... 73
3.2.5 Non-Dimensionalisation ...... 74
3.2.6 Non-Dimensional Boundary Conditions ...... 74
3.2.6.1 Periodicity in x ...... 74
3.2.6.2 Conditions at y =0 ...... 75
3.2.6.3 Large y Behavior ...... 76
3.3 Idealised Model of LDL Transport ...... 76
3.3.1 Domain and Governing Equation ...... 76
3.3.2 Suitable Definition of Macroscale LDL Concentration Polari- sation Layer ...... 76
3.3.3 Non-Dimensionalisation ...... 77
3.3.4 Non-Dimensional Boundary Conditions ...... 79
3.3.4.1 Periodicity in x ...... 79
3.3.4.2 Condition at y =0...... 79
13 3.3.4.3 Condition at y = Lα ...... 80
3.4 Implementation ...... 82
3.4.1 Water Velocity Field ...... 82
3.4.1.1 Formulating in Terms of a Stream Function . . . . . 82
3.4.1.2 Trial Solution for ψα ...... 82
3.4.1.3 Application of Boundary Conditions ...... 82
3.4.1.4 Velocity Field Solution ...... 83
3.4.2 LDL Concentration Field ...... 83
3.4.3 Parameter Values ...... 84
3.4.3.1 Value for the Non-Dimensional Cleft Half-Width δ . 84
3.4.3.2 Values for the Non-Dimensional Shear Rate γ .... 85
3.4.3.3 Values for the Peclet Number P eL ...... 85
3.4.3.4 Value for the Non-Dimensional Height Lα of ΩαC .. 86
3.5 Results and Analysis ...... 86
3.5.1 Water Velocity Field ...... 86
3.5.2 LDL Concentration Field ...... 87
3.5.3 Transendothelial LDL Transport ...... 91
3.5.3.1 Definitions ...... 91
3.5.3.2 Dependence of CαU and CαN on P eL ...... 92
3.5.3.3 Dependence of CαU and CαN on γ ...... 94
3.5.4 Extending the Parameter Space ...... 96
14 3.5.5 Implications of Neglecting Tight Junction Strands ...... 100
3.5.6 Implications of Neglecting Pulsatile Blood Flow ...... 100
3.6 Conclusions ...... 101
4 The Effect of an Endothelial Glycocalyx Layer 102
4.1 Overview of Idealised Model ...... 102
4.2 Idealised Model of Water Flow ...... 103
4.2.1 Heterogeneous Transmural Flux and Applied Shear ...... 103
4.2.2 Domain and Governing Equations ...... 103
4.2.3 Non-Dimensionalisation ...... 106
4.2.4 Non-Dimensional Boundary Conditions ...... 108
4.2.4.1 EGL/Lumen Interface ...... 108
4.2.4.2 Periodicity in x ...... 109
4.2.4.3 Conditions at y =0 ...... 109
4.2.4.4 Large y Behavior ...... 110
4.3 Idealised Model of LDL Transport ...... 110
4.3.1 Domain and Governing Equation ...... 110
4.3.2 Suitable Definition of Macroscale LDL Concentration Polari- sation Layer ...... 112
4.3.3 Non-Dimensionalisation ...... 113
4.3.4 Non-Dimensional Boundary Conditions ...... 115
4.3.4.1 Periodicity in x ...... 115
15 4.3.4.2 Condition at y = h − b ...... 115
4.3.4.3 Condition at y = h − b + L ...... 115
4.4 Implementation ...... 117
4.4.1 Water Velocity Field ...... 117
4.4.1.1 Formulating in Terms of Stream Functions ...... 117
4.4.1.2 Trial Solution for ψβL ...... 118
4.4.1.3 Trial Solution for ψβG when Dax ≤ Day ...... 118
4.4.1.4 Trial Solution for ψβG when Dax > Day ...... 119
4.4.1.5 Application of Boundary Conditions ...... 120
4.4.1.6 Velocity Field Solution ...... 123
4.4.2 LDL Concentration Field ...... 124
4.4.3 Parameter Values ...... 125
4.4.3.1 Value for the Non-Dimensional Cleft Half-Width δ . 125
4.4.3.2 Values for the Non-Dimensional Shear Rate γ .... 125
4.4.3.3 Values for Cleft Peclet Number P eL ...... 125
4.4.3.4 Values for the Non-Dimensional EGL Height h ... 125
4.4.3.5 Values for the Non-Dimensional Darcy Permeabili-
ties Dax and Day ...... 126
4.4.3.6 Values for the Ratio of EGL to Lumen LDL Diffu-
sivity Dr ...... 126
4.4.3.7 Values for the Non-Dimensional Distance b that LDL Penetrates into the EGL ...... 126
16 4.4.3.8 Value for the Non-Dimensional Height Lβ of ΩβC .. 127
4.5 Results and Analysis ...... 127
4.5.1 Water Velocity Field ...... 127
4.5.1.1 Streamlines ...... 127
4.5.1.2 Wall Normal Velocity ...... 129
4.5.2 LDL Concentration Field (No LDL Penetration into the EGL) 130
4.5.3 Transendothelial LDL Transport (No LDL Penetration into the EGL) ...... 133
4.5.3.1 Definitions ...... 133
4.5.3.2 Dependence of CβU and CβN on Applied Shear γ .. 135
4.5.3.3 Dependence of CβU and CβN on EGL Properties h,
Dax and Day ...... 135
4.5.4 LDL Concentration Field (LDL Penetration into the EGL) . . 135
4.5.5 Transendothelial LDL Transport (LDL Penetration into the EGL) ...... 141
4.5.5.1 Dependence of CβU and CβN on Applied Shear γ .. 141
4.5.5.2 Dependence of CβU and CβN on LDL Interaction
with the EGL (h, b and Dr)...... 141
4.6 Conclusions ...... 145
5 Conclusions and Future Research 146
5.1 Conclusions ...... 146
5.2 Future Research ...... 147
17 5.2.1 Future Theoretical Research ...... 147
5.2.2 Future Experimental Research ...... 149
Bibliography 150
A Applicability 160
B Convergence 162
C Time Dependent Simulations 164
C.1 Water Velocity Field ...... 164
C.2 LDL Concentration Field ...... 165
C.3 Transendothelial LDL Transport ...... 166
C.4 Results ...... 167
D Trial Solution for ψβG when Dax > Day 168
ˆ ˆ ˆ ˆ ˆ ˆ E Explicit Expressions for Aβn, Bβn, Cβn, Dβn, Eβn and Fβn 171
F Resulting Publications and Presentations 179
F.1 Journal Articles ...... 179
F.2 Conference Contributions ...... 180
F.3 Seminars ...... 182
18 List of Figures
1.1 Schematic illustration of the interface between the arterial wall and the lumen...... 30
1.2 Diagram illustrating how concentration polarisation of a solute can occur adjacent to a generic membrane...... 34
1.3 Schematic illustration of LDL concentration polarisation adjacent to the luminal surface of the arterial endothelium...... 36
1.4 Schematic illustration of a tight junction strand within an intercellu- lar cleft...... 38
1.5 Illustration of EGL structure...... 39
1.6 Image of the EGL within a rat ventricular myocardial capillary ob- tained using electron microscopy...... 40
2.1 Graphical illustration of global spectral/hp basis functions...... 50
2.2 A quadrangular standard element...... 59
2.3 A triangular standard element...... 60
3.1 Idealisation of intercellular cleft pattern...... 70
3.2 Idealised periodically repeating domains ΩαV and ΩαC adjacent to the endothelial surface...... 73 ∗ 3.3 Schematic illustration of Cα...... 77
3.4 Computational mesh of the domain ΩαC ...... 84
3.5 Velocity streamlines in the vicinity of an intercellular cleft...... 87
3.6 Contour plots of Cα...... 88
3.7 Plots illustrating how the LDL distribution adjacent to the endothe- lium varies with γ...... 89
3.8 Plots of CαU and CαN against P eL...... 92
3.9 Plots of (CαU − 1) against P eL...... 94
3.10 Plots of CαU and CαN against γ...... 95
3.11 Plots of (CαU − 1) and (CαN − 1) against δ...... 97
3.12 Plots of CαU against γ for various values of δ...... 98
3.13 Plots of CαU against P eL and (CαU -1) against P eL...... 99
4.1 Idealised periodically repeating domain ΩβV ...... 104
4.2 Idealised periodically repeating domain ΩβC ...... 111
∗ 4.3 Schematic illustration of Cβ...... 113
4.4 Computational mesh of the domain ΩβC ...... 124
4.5 Velocity streamlines in the vicinity of an intercellular cleft...... 128
4.6 Plots of the wall normal velocity at the luminal surface of the EGL. . 129
4.7 Plots illustrating how the LDL distribution adjacent to the luminal surface of the EGL varies with EGL height h for cases where LDL cannot penetrate into the EGL...... 131
20 4.8 Plots illustrating how the LDL distribution adjacent to the luminal
surface of the EGL varies with Dax and Day for cases where no LDL can penetrate into the EGL...... 132
4.9 Contour plots of Cβ...... 137
4.10 Plots illustrating how the LDL distribution evaluated at y = 0.05 − b varies with b for cases where LDL can penetrate a distance b into an EGL of height h = 0.05...... 139
4.11 Plots illustrating how the LDL distribution evaluated at y = 0.1 − b varies with b for cases where LDL can penetrate a distance b into an EGL of height h = 0.1...... 140
4.12 Plots of CβU and CβN against b for the case where LDL can penetrate a distance b into an EGL of height h = 0.05...... 142
4.13 Plots of CβU and CβN against b for the case where LDL can penetrate a distance b into an EGL of height h = 0.1...... 143
∗ ∗ A.1 Plot of CEm/CB against γ...... 161
B.1 Plots of EM against M...... 163
21 List of Tables
4.1 Ranges of CβU and CβN as LDL penetration distance varies over the range b = 0.01 − 0.05...... 144 Chapter 1
Introduction
1.1 Atherosclerosis
1.1.1 Overview
Atherosclerosis is a common disease of the human vascular system, characterised by the formation of lipid-rich lesions within the walls of large arteries. After several decades of growth such lesions may act to stenose their native vessel, leading to symptoms such as angina (caused by coronary stenoses restricting blood flow to the heart). Further to causing stenoses, lesions may also become unstable and hence prone to rupture. When an atherosclerotic lesion ruptures a mass of thrombogenic material is released into the lumen, causing a blood clot to form. Such a clot may cause sudden and complete arterial occlusion, and hence severe disruption of the oxygen supply to organs within the body. Two well known consequences of such occlusion are heart attacks (caused by occlusion of a coronary artery), and strokes (caused by occlusion of an artery that supplies the brain). In addition to its severe consequences, atherosclerosis is also striking in its worldwide prevalence. According to the World Health Organisation (WHO) cardiovascular disease, and in particular atherosclerosis, is now the leading cause of death globally each year [1]. Furthermore, by 2020 the WHO predict that atherosclerosis will become the single most burdensome disease on the health systems of the world [2].
1.1.2 Initiation of Atherosclerosis
This thesis is primarily concerned with the initiation of atherosclerosis, as opposed to processes involved in the later stages of the disease. At a simplistic level the most fundamental steps involved in the early stages of atherosclerosis development can be outlined as follows:
• Low Density Lipoproteins (LDL), which are the primary transporter of choles- terol within the blood, begin to accumulate in the intima of the arterial wall. Accumulated LDL becomes modified (oxidised for example), and re- leases chemicals that attract monocytes to the regions of LDL build up.
• Monocytes enter the vascular wall at sites of LDL accumulation and differ- entiate into macrophages. These macrophages ingest the accumulated LDL, creating lipid-rich foam cells.
• Mechanisms involving High Density Lipoproteins (HDL), for example, can act to remove accumulated lipids from foam cells.
• If lipid influx into the arterial wall is consistently greater than lipid efflux from the wall, then a net accumulation of lipid-rich foam cells will begin to occur.
• This unchecked net accumulation of lipid-rich foam cells is a marker of an early stage atherosclerotic lesion.
The outline of the atherosclerosis initiation process presented above is generally accepted in the literature [3, 4]. What remains contentious, however, are the mech- anisms by which the process is regulated i.e. what promotes and what limits its occurrence.
24 1.1.3 Inter-Human Variation
The fact that not all humans exhibit pathological atherosclerosis indicates that its development is regulated at an inter-human level (i.e. between humans). It is observed that the disease develops preferentially in individuals exhibiting a range of risk factors. The most important of these risk factors are listed below:
• High levels of LDL in the blood.
• Low levels of HDL in the blood.
• High blood pressure.
• Diabetes.
• Smoking.
• Gender (being male).
• Genetic predisposition.
• Excess stress.
• Lack of exercise.
Generally, the factors in the above list have been identified empirically. They offer some useful insight into the process of atherosclerosis initiation. However, they do not allow detailed elucidation of any processes that regulate onset of the disease.
1.1.4 Intra-Human Variation
As well as varying between individuals, the prevalence of atherosclerotic lesions is also seen to vary at the intra-human level (i.e. within the arterial vasculature), with lesions developing preferentially in regions of arterial branching and high curvature. Since these particular regions are associated with complex blood flow patterns, it
25 has been postulated that blood flow, which is also spatially heterogeneous at the vascular scale, may play an important role in regulating atherogenesis [5, 6]. Sev- eral mechanisms that could lead to a flow dependence of atherogenesis have been suggested. Such mechanisms will be discussed in more detail shortly.
A fuller understanding of the mechanisms that cause atherosclerosis to be spatially heterogeneous could lead to a fuller understanding of the mechanisms that regulate onset of atherosclerosis per se. Such enhanced understanding could potentially lead to the development of improved therapies to avert or treat the disease.
1.2 Blood Flow and Atherosclerosis
1.2.1 Overview
Correlations between blood flow patterns and sites of arterial disease have been suggested for over a century. One of the earliest proponents of such correlations was Rindfleisch, who in 1872 stated that atherosclerotic lesions formed in locations ‘exposed to the full stress and impact of the blood’ [7]. Based on the observations of Rindfleisch, although almost 100 years after they were initially made, a variety of mechanisms to explain correlations between flow and disease were proposed during the 1960’s. Generally, such mechanisms relied on flow induced wall damage ren- dering particular regions of the vasculature more permeable to atherogenic species such as LDL, and thus more susceptible to atherosclerosis [8]. As a consequence of these initial theories, a general consensus developed by the end of the 1960’s that regions exposed to high levels of wall shear stress were predisposed to developing atherosclerosis [9].
In the late 1960’s and early 1970’s, however, two papers by Caro et al. overturned the previously held consensus that high levels of wall shear stress were atherogenic. Caro et al. instead suggested that regions of arterial disease were colocated with areas exposed to low levels of wall shear stress [10, 11]. Furthermore, Caro et al. also
26 proposed a mechanism by which such colocation could occur. This mechanism was more sophisticated than any previously suggested, and relied on the shear modulated efflux of species (such as LDL) from the arterial wall into the lumen.
After its conception in the early 1970’s, the low shear hypothesis of Caro et al. became widely accepted. To a large extent, the idea that lesions develop at sites of low wall shear stress is still accepted today (although the original mechanism proposed by Caro et al. to cause such colocation is now considered unfeasible). In recent decades, however, it has become increasingly evident that a direct correla- tion between disease patterns and (solely) wall shear stress magnitude may be too simplistic. A wide range of more complex relationships have been suggested, with a tentative consensus now developing that a combination of low and temporally oscillating wall shear stress predisposes regions of arteries to disease [12, 13, 14]. An array of mechanisms attempting to explain these more complex relationships have also been suggested. Such mechanisms generally, although not always, fall into one of two categories. The first category contains mechanisms whereby mechani- cal forces due to blood flow directly influence properties of the arterial wall [15], whereas the second category contains mechanisms reliant on the flow dependent transport of species to, into, and out of the arterial wall [16, 17]. Mechanisms from either category often have interlinking components, and the implications of individ- ual mechanisms often overlap. The current picture is thus highly complex. Brief overviews of each type of mechanism are given below.
Before proceeding with discussions, it is important to highlight the following salient point. It is not being suggested that atherosclerosis occurs solely because individuals develop atherogenic blood flow patterns. Rather it is being suggested that blood flow predisposes certain regions of the vasculature to atherosclerosis (when the disease is induced by the risk factors mentioned in section 1.1.3). This point was also noted over 100 years ago by Rindfleisch, who stated that ‘mechanical irritation must not be regarded as the sole cause of the disorder, though it determines its localisation. Among other predisposing causes are advanced age and free living’ [7].
27 1.2.2 Regulation by Mechanical Forces
The luminal surface of the arterial wall is lined with a monolayer of endothelial cells, known collectively as the endothelium. The endothelium is likely to play a key role in the process of atherogenesis, since it acts as a barrier [18] between the luminal blood (containing LDL and monocytes) and the intima (where atherosclerotic lesions begin to develop).
It has been demonstrated that the endothelium is able to sense applied flow forces, and respond in various ways. One well know example of such a response is the observed alignment of vascular endothelial cells with the direction of blood flow [19, 20]. There is currently much debate regarding exactly how endothelial cells sense and respond to applied forces. A wide range of mechano-chemical transducers have been implicated in the process, including flow activated ion channels, tyrosine kinase receptors, G proteins, cell-cell junction molecules and the endothelial gly- cocalyx layer. These transducers are currently associated with a vast array of flow dependent endothelial responses [15, 21, 22], a detailed review of which is beyond the scope of this thesis. Suffice it to say that many of the responses may affect arterial susceptibility to atherosclerosis (by varying endothelial permeability to atherogenic species for example). Therefore, endothelial mechano-chemical transduction mech- anisms constitute a direct way in which mechanical forces, and hence blood flow patterns, could regulate the onset of arterial disease.
1.2.3 Regulation by Mass Transport Mechanisms
Several cells/species are thought to play key roles in the process of atherosclerosis initiation. LDL, HDL, and monocytes have already been mentioned, since they are likely to play a fundamental role. Other important species include oxygen (O2), ni- tric oxide (NO), adenosine triphosphate (ATP), and adenosine diphosphate (ADP). It has been postulated that blood flow patterns may regulate transport of several of the aforementioned species to, into and out of the arterial wall. Such flow depen-
28 dent species transport could offer an explanation for the observed flow dependence of atherosclerosis.
There have been a range of experimental and numerical studies investigating O2 [23], ATP, ADP [24] and LDL [25, 26, 27, 28] transport within arteries. A review of computational modelling techniques applied to arterial mass transport is given by Ethier [16], and a review of arterial mass transport in general (with a particular focus on its relation to the localisation of atherosclerosis) is given by Tarbell [17]. The review of Tarbell splits arterial mass transport processes into two distinct groups, namely those termed ‘fluid-phase-limited’ and those termed ‘wall-limited’. Broadly speaking these two types of process can be described as follows:
• Fluid-phase-limited processes are those in which the rate of species transport into the arterial wall is limited by the rate at which species are transported to the wall from the flowing blood. It has been suggested that low molecular
weight species that react quickly with the arterial wall (such as O2 and ATP) enter the arterial wall in a fluid-phase-limited fashion [17].
• Wall-limited processes are those in which the rate of species transport into the arterial wall is limited by the wall itself, not by a fluid-phase-limited trans- port process. It has been suggested that high molecular weight species that are offered significant resistance by the arterial wall (such as LDL) enter the arterial wall in a wall-limited fashion [17].
For a fluid-phase-limited transport process, it is clear that blood flow patterns may control the rate of species uptake by the arterial wall (potentially causing flow de- pendent regulation of atherogenesis). For wall-limited transport processes, however, the situation is less clear. It is often implied that wall-limited processes will be flow-independent (simply because they are independent of fluid-phase transport). Indeed the terms wall-limited and flow-independent are often used synonymously. For a variety of reasons, however, such synonymous use of these terms is not nec- essarily correct. As an illustrative example of why wall-limited does not necessarily
29 mean flow-independent, consider specifically the process of transendothelial LDL transport. It has been suggested that this process is independent of fluid-phase transport and hence wall-limited [17], with the argument as to why proceeding in the following manner [17, 29].
Consider LDL transport within the locality of an arbitrary point on the arterial wall (as illustrated in Fig. 1.1).
Endothelium
Arterial Lumen Wall Artery
* * * CW CE CB
* * kE kB
Figure 1.1: Schematic illustration of the interface between the arterial wall and ∗ the lumen. LDL concentration in the arterial wall is denoted CW , LDL concentra- ∗ tion adjacent to the luminal surface of the endothelium is denoted CE, and LDL ∗ concentration in the bulk flow is denoted CB (all within the locality of an arbitrary point on the arterial wall). The endothelium is considered to have a permeability ∗ kE to LDL. It is assumed that fluid-phase LDL transfer from the bulk flow to the ∗ endothelial surface is characterised by a mass transfer coefficient kB.
Further, consider that the flux of LDL across the endothelium into the arterial wall
∗ JE is given by
∗ ∗ ∗ ∗ JE = kE(CE − CW ), (1.1)
∗ where CE is the LDL concentration adjacent to the luminal surface of the endothe-
30 ∗ lium, CW is the LDL concentration on the abluminal surface of the endothelium ∗ (in the arterial wall), and kE is the permeability of the endothelium to LDL. Also, consider that the flux of LDL from the flowing blood to the luminal surface of the
∗ endothelium JB is given by
∗ ∗ ∗ ∗ JB = kB(CB − CE), (1.2)
∗ ∗ where CB is the LDL concentration in the bulk blood flow, and kB is a blood side mass transfer coefficient. The review of Tarbell [17] (from which the present analysis
∗ is taken) states that kB characterises a convective-diffusive LDL transport mecha- nism. This statement is true, although slightly misleading, since due to the form of
∗ ∗ Eq. (1.2) JB can only explicitly model diffusional LDL transport. Therefore, kB only accounts for convection insomuch as it accounts for its effect on the thickness and form of the LDL concentration boundary layer (and thus on the diffusional transport
∗ of LDL to the endothelial surface). The mass transfer coefficient kB, and hence the present analysis, cannot directly account for any convective LDL transport towards the endothelium. The implications of this limitation will be discussed shortly. For now, however, we return to the analysis and assume that in steady state
∗ ∗ JB = JE. (1.3)
Further, it is assumed that since the endothelium offers a significant resistance to LDL
∗ ∗ CW CE. (1.4)
∗ Substituting Eq. (1.1) and Eq. (1.2) into Eq. (1.3), and setting CW = 0 due to Eq. (1.4), one obtains
∗ ∗ ∗ ∗ ∗ kB(CB − CE) = kECE, and hence
31 ∗ ∗ CB CE = ∗ ∗ . (1.5) 1 + (kE/kB)
∗ ∗ Finally, it is assumed that for LDL kE kB, hence Eq. (1.5) can be re-written as
∗ ∗ CE = CB. (1.6)
Eq. (1.6) indicates that LDL concentration adjacent to the luminal surface of the
∗ ∗ endothelium CE is likely to be independent of kB, and hence independent of fluid- ∗ phase transport processes. The implication of this result is that JE (which is given ∗ ∗ by CBkE under the above assumptions) is also likely to be independent of fluid-phase transport. Transendothelial LDL transport is therefore deemed to be a wall-limited process.
Although the above analysis indicates that transendothelial LDL transport is inde- pendent of fluid-phase LDL transport, it has not shown the process to be completely flow-independent. There are in fact three ways in which blood flow could control the rate of LDL transport across the endothelium. The first two mechanisms can be understood within the context of the above analysis, and can be described as follows:
• Flow could regulate endothelial permeability to LDL via a mechanochemical transduction mechanism (as described in Section 1.2.2). Such flow-dependent modulation of endothelial permeability would clearly cause the transendothe- lial LDL flux to become flow dependent.
• A fluid-phase-limited mass transfer process (of a species such as O2) could regulate endothelial permeability to LDL. Such flow-dependent modulation of endothelial permeability would clearly cause the transendothelial LDL flux to become flow dependent.
The third and final mechanism, however, cannot be understood within the context of the above analysis, since it relies on the existence of a wall-normal convective LDL
32 flux, which (as has been discussed) cannot be explicitly represented by Eq. (1.2). It has been postulated that such a wall normal convective flux will cause flow- dependent LDL concentration polarisation to occur adjacent to the luminal surface of the endothelium. Details of this final mechanism are given in the following section.
1.3 Flow Dependent LDL Concentration Polari- sation within Arteries
1.3.1 Concentration Polarisation
Consider a fluid containing a dissolved solute flowing through a membrane. If the membrane offers a higher resistance to the solute than the fluid, then solute will be rejected by the membrane and accumulate on its upstream surface. It is this process of solute accumulation that is referred to as concentration polarisation. The layer of rejected solute is often referred to as a concentration polarisation layer (see Fig. 1.2). As concentration polarisation occurs a concentration gradient will develop, causing solute to diffuse back away from the membrane (in the opposite direction to the approaching fluid flow). A steady state solute distribution is reached when solute convection towards the membrane balances with solute diffusion away from the membrane and solute transport across it.
33
Convection
Diffusion Fluid
Solute
Concentration Polarisation Layer
Membrane Transport Across Membrane
Figure 1.2: Diagram illustrating how concentration polarisation of a dissolved solute can occur adjacent to a generic membrane from which the solute is fully or partially rejected. A steady state is reached when convection towards the membrane (solid arrow) balances with diffusion away from the membrane (checkered arrow) and transport across the membrane (striped arrow).
The phenomenon of concentration polarisation is well known within various fields of science and engineering, in particular those involving filtration processes.
1.3.2 LDL Concentration Polarisation within Arteries
LDL concentration polarisation is postulated to occur in arteries due to the trans- mural water flux that flows radially outwards (from the lumen) through the arte- rial wall. There is an imbalance between the measured velocity of this water flux (∼ 4 × 10−2 µms−1 [30]) and the measured permeability of the endothelium to LDL (∼ 2×10−4 µms−1 [31]). Due to this imbalance LDL convection towards the luminal surface of the endothelium is likely to be far greater that the rate of transendothelial LDL transport, resulting in the formation of an LDL-rich (concentration polarisa- tion) layer adjacent to the endothelial surface.
34 1.3.3 Flow Dependent LDL Concentration Polarisation within Arteries
Consider the formation of an LDL concentration polarisation layer within the local- ity of an arbitrary point adjacent to the luminal surface of the arterial wall. Further, consider defining a wall normal coordinate y∗ at this arbitrary point of interest (see Fig. 1.3). When modelling LDL transport above the endothelium it can be assumed that LDL is completely rejected from the endothelial surface (since endothelial per- meability to LDL is likely negligible c.f. the transmural water flux). If it is assumed that LDL is rejected from the endothelium at y∗ = R∗ (where R∗ is arbitrary and introduced for later convenience), then lumen side convection and diffusion must balance at y∗ = R∗, and hence
∗ ∂C ∗ ∗ D∗ (R∗) = −V C (R∗), (1.7) L ∂y∗
∗ ∗ where DL is the diffusivity of LDL in the lumen and V is the magnitude of the transmural flux velocity (assumed to flow in the negative y∗ direction towards the endothelial surface).
Given the condition defined by Eq. (1.7), and assuming that the concentration po- larisation layer can be modelled locally as a stagnant film [32, 33], convection and diffusion must balance along the y∗ coordinate within the concentration polarisa- ∗ tion layer. Hence, the y∗ dependent LDL distribution C within the concentration polarisation layer is a solution of
∗ ∂C ∗ ∗ D∗ = −V C . (1.8) L ∂y∗
In order to solve Eq. (1.8) a single boundary condition is required. To obtain such a condition it is assumed that the concentration polarisation layer has a finite thickness ζ∗ within the locality of the arbitrary point of interest (see Fig. 1.3), where ζ∗ is dependent upon the local haemodynamics. If (as before) LDL concentration
∗ in the bulk flow is denoted CB, then the above assumption requires that
35 ∗ ∗ ∗ ∗ C (R + ζ ) = CB. (1.9)
On solving Eq. (1.8) subject to the boundary condition defined by Eq. (1.9), one obtains the following revised expression for the LDL concentration adjacent to the
∗ luminal surface of the endothelium CE (at the arbitrary point of interest)
∗ ∗ ∗ ∗ ∗ (V ζ /DL) CE = CBe , (1.10)
∗ along with the following expression for the LDL distribution C within the concen- tration polarisation layer (i.e. within the region R∗ < y∗ < R∗ +ζ∗) at the arbitrary point of interest
∗ ∗ ∗ ∗ ∗ ∗ −V (y −R )/DL C = CEe . (1.11)
The concentration polarisation layer defined by Eq. (1.11) will henceforth be referred to as the ‘macroscale LDL concentration polarisation layer’ (at the arbitrary point of interest).
C*
* CE Lumen Artery
y*
* CB !* * 0 R* R*+!* y
Figure 1.3: Schematic illustration of LDL concentration polarisation adjacent to the luminal surface of the arterial endothelium. It is assumed that the concentration polarisation layer has a flow dependent thickness ζ∗. Further, it is assumed that LDL is rejected from the endothelium at y∗ = R∗, where R∗ is arbitrary and introduced for later convenience.
36 Eq. (1.10) can be compared directly with Eq. (1.6) (which was obtained via a more simplistic analysis that ignored the effect of the transmural water flux). The
∗ important point to note is that CE given by Eq. (1.10) is dependent on local ∗ ∗ haemodynamics (via its dependence on ζ ), whereas CE given by Eq. (1.6) does not depend on flow. Consideration of the transmural water flux has revealed a mechanism by which flow can control the degree of endothelial exposure to LDL.
1.3.4 Flow Dependent Regulation of Atherogenesis
The route by which LDL crosses the endothelium and enters the arterial wall is not known definitively. It is observed, however, that increasing plasma LDL concentra- tion (and hence endothelial exposure to LDL) increases the rate of transendothelial LDL transport [34]. Such a finding implies that the degree of LDL concentration polarisation could act to modulate the rate of LDL transport into the intima, and thus the likelihood of atherosclerosis occurring. If (as suggested above) the local degree of LDL concentration polarisation is dependent on vascular scale flow fea- tures, then the above mechanism provides a viable explanation for the observed flow dependence of atherogenesis [35, 36].
1.3.5 Previous Studies
Experiments suggest that a flow dependent LDL concentration polarisation layer does form within the vasculature [25, 26]. These experimental results are supported by vascular scale theoretical studies [27, 28], which also quantify how the degree of concentration polarisation might depend on vascular scale flow features. It is the case, however, that these previous studies have generally overlooked several cellular scale features of the endothelial surface. In particular they have not accounted for the fact that the transmural water flux is likely to be spatially heterogeneous as it crosses the endothelium [37]. Also, they have not accounted for the fact that an endothelial glycocalyx layer covers the luminal surface of endothelial cells [38, 39].
37 1.4 Relevant Cellular Scale Features of the En- dothelial Surface
1.4.1 Spatially Heterogeneous Transmural Water Flux
Blood plasma consists of approximately 92% water. Studies of capillaries suggest that the water component of blood plasma traverses the endothelium predominantly via intercellular clefts (between endothelial cells) [37] rather than through the en- dothelial cells themselves. Therefore the transmural water flux is likely to be spa- tially heterogeneous at the cellular scale as it crosses the endothelium. Further studies of capillaries reveal that within intercellular clefts there exists a complex structure of connections referred to as tight junction strands [40]. These are thought to form a disjointed barrier around almost the entire cell periphery (see Fig. 1.4), with the passage of water occurring preferentially at locations where the junction strands are broken. Such structures within the depth of each intercellular cleft may result in further spatial localisation of the transmural water flux as it crosses the endothelium [41].
Tight Junction Strand Break in Tight Junction Strand
Intercellular Cleft Entrance
Endothelial Cell
Endothelial Cell
Figure 1.4: Schematic illustration of a tight junction strand within an intercellular cleft. Note that the strands are broken at particular locations.
38 Previous review articles [16, 17] have stated that a heterogeneous transmural water flux is likely to affect LDL concentration polarisation within the vasculature. How- ever, the precise nature of such an effect and its influence on the flow-dependent entry of LDL into the arterial wall have not been established, and are not intu- itively obvious. The problem has been addressed by one earlier numerical study [42]. This study, however, did not use realistic intercellular cleft dimensions, nor did it fully investigate a realistic range of LDL diffusivities.
1.4.2 Endothelial Glycocalyx Layer
Attached to the luminal surface of vascular endothelial cells, and likely covering the intercellular clefts, is a structure known as the endothelial glycocalyx layer (EGL). The EGL is currently understood to be formed of two distinct yet closely interacting regions [38, 39] as illustrated in Fig. 1.5.
Lumen
(b) ~ 0.5 µm EGL
0.05-0.4 µm (a)
Endothelial Cell
Figure 1.5: Illustration of EGL structure (not to scale). It is thought that the EGL is composed of a well adhered layer of long chain macromolecules extending ∼ 0.05−0.4µm from the endothelial surface (a) and a more dynamic loosely attached layer of endothelial and plasma derived macromolecules (b), which act to extend the EGL ∼ 0.5 − 1.0µm into the lumen.
The first layer (Fig. 1.5 label (a)) is composed of long chain macromolecules (pre- dominantly proteoglycans and glycoproteins) firmly attached to the luminal surface of the underlying endothelial cells. This region of the EGL is often observed in
39 ex-vivo electron microscope studies (see Fig. 1.6), and extends ∼ 0.05 − 0.4µm [43] from the cell surface. The second layer (Fig. 1.5 label (b)) is thought to be more dynamic in nature, composed of loosely attached plasma and endothelial derived proteins which act to extend the EGL ∼ 0.3−0.5µm [44, 45, 46] (or possibly further [47]) into the lumen.
Figure 1.6: Image of the EGL within a rat ventricular myocardial capillary ob- tained using electron microscopy. Reused with permission from B. M. van den Berg et al. [48]. Copyright 2003, Wolters Kluwer Health.
The EGL is postulated to play an important role in several processes, including the prevention of red blood cell interaction with the endothelium [49] and the transduc- tion of mechanical forces to the surface of endothelial cells [50]. It is the role of the EGL as a macro-molecular sieve [51], however, that is most likely to have an effect on LDL concentration polarisation within arteries. Specifically, the distance that LDL can penetrate into the EGL will determine the local water velocity profile and LDL diffusivity close to the endothelium, both of which are important determinants of the structure and degree of any LDL concentration polarisation that occurs.
It can be noted that the EGL (as described above) is sometimes referred to simply as the ‘glycocalyx’ or alternatively the ‘endothelial surface layer’ [52]. To add fur- ther confusion, the well adhered layer of macromolecules at the base of the EGL is
40 sometimes referred to alone as the glycocalyx (since this region was the first to be regularly observed). To avoid such confusions the term EGL is adopted consistently throughout this thesis to refer to the entire structure described above. Individual regions of the EGL are referred to explicitly when necessary.
Overviews of the structure and function of the EGL are given in recent review articles by Weinbaum et al. [38] and Reitsma et. al. [39].
1.5 Objective of Thesis
The objective of this thesis is to assess the effect of a heterogeneous transmural water flux and an EGL on LDL concentration polarisation in arteries. Particular attention is paid to measures of LDL concentration polarisation relevant to the rate of transendothelial LDL transport, since this rate has implications for the likelihood of atherosclerosis onset.
1.6 Overview of Thesis
In Chapter 2 an overview is given of the numerical scheme that will be used through- out this thesis (namely the spectral/hp element method). Particular attention is focused on obtaining numerical solutions to the two-dimensional (2D) steady and unsteady advection diffusion equations. In Chapter 3 an idealised model is devel- oped and implemented in order to assess the effect of a heterogeneous transmural water flux on LDL concentration polarisation in arteries (published in Biophysical Journal [53]). In Chapter 4 this model is extended to include the effect of the EGL (published in Physics of Fluids [54], and submitted for publication in Journal of Theoretical Biology). Finally, in Chapter 5 conclusions and ideas for future research are presented.
41 Chapter 2
Spectral/hp Element Method
2.1 Overview
It is often difficult, and in some cases impossible, to derive analytical solutions to a differential equation. The applicability of analytical techniques is therefore somewhat limited. As a consequence, a range of numerical methods have been developed in order to obtain approximate solutions to differential equations. Such numerical techniques have a wide range of applicability, and are hence currently employed in numerous fields of science and engineering.
There are several well known types of numerical method. These include finite dif- ference methods [55], finite volume methods [56], finite element methods [57] and spectral methods [58], each of which has its own advantages and disadvantages when applied to particular problems. Numerous implementations and variations of the aforementioned methods have been developed. A spectral/hp element method [59] can be viewed as an implementation of a finite element scheme in which the principles of spectral methods are also employed.
When implementing a finite element method, the domain of interest is decomposed spatially into separate regions known as elements. The solution is then represented within each element of the domain using a polynomial function (which is often sim- ply linear). Such decomposition is often referred to as h-type discretisation, and increasing the number of elements is often referred to as h-type refinement. The spatial discretisation employed when using a finite element method does not have to be uniform, hence finite element techniques lend themselves well to problems in which the geometry is complex. Also, due to the flexibility of the spatial discretisa- tion, elements (and hence degrees of freedom) can be localised in particular regions of the domain. The ability to spatially localise degrees of freedom can be extremely useful if one has a priori knowledge of where complex features of the solution may develop.
When implementing a spectral method the solution is decomposed in frequency space into modes, which are defined globally within the domain of interest. Such decomposition is often referred to as p-type discretisation, and increasing the num- ber of modes is often referred to as p-type refinement. Spectral methods lack the geometrical flexibility of finite element methods, since it is often difficult to define continuous global modes within complex geometries. However, in geometries where spectral methods can be applied they are known to exhibit excellent convergence properties. Specifically, if the solution is smooth then spectral methods will converge exponentially as the number of modes (degrees of freedom) is increased. This can be compared with the algebraic convergence exhibited by finite element methods as the number of elements (degrees of freedom) is increased.
The principle of spectral/hp element methods is to combine the geometrical flexi- bility of finite element methods with the superior convergence properties of spectral methods. This is achieved by decomposing the domain of interest spatially into ele- ments (h-type discretisation), and then representing the solution within each element using a summation of modes (p-type discretisation). A particular implementation of the spectral/hp element method will be employed in Chapters 3 and 4 to find approximate solutions of the 2D steady and unsteady advection diffusion equations. The main principles of the method are outlined below.
43 2.2 One-Dimensional Spectral/hp Element Method
2.2.1 Example Problem
For illustrative purposes, consider the inhomogeneous one-dimensional (1D) Helmholtz equation d2u − λu = f, (2.1) dx2 where u = u(x) is a scalar field, f = f(x) is a forcing function, and λ is a real positive constant. Further, consider finding a solution of Eq. (2.1) within the domain Ω = {x | x0 ≤ x ≤ x4}, that satisfies the following boundary conditions
u(x0) = gD, (2.2)
du (x ) = g , (2.3) dx 4 N where gD and gN are known constants. Eq. (2.1), along with the boundary con- ditions defined by Eq. (2.2) and Eq. (2.3), are said to pose the problem in its strong form (as opposed to in its weak form which will be discussed shortly). It can be noted that in the above example the boundary condition applied at x = x0 is a condition on the solution (often referred to as a Dirichlet boundary condition), whereas the boundary condition applied at x = x4 is a condition on the derivative of the solution (often referred to as a Neumann boundary condition).
2.2.2 Weak Formulation
If Eq. (2.1) is multiplied through by an arbitrary test function v = v(x) (defined to be zero on all Dirichlet boundaries), and then integrated over the whole domain, the following expression is obtained
Z x4 d2u Z x4 Z x4 v 2 dx − λ vu dx = vf dx. x0 dx x0 x0
44 Integration by parts leads to
x4 Z x4 Z x4 Z x4 du dv du v − dx − λ vu dx = vf dx, dx dx dx x0 x0 x0 x0 and hence
Z x4 dv du Z x4 du du Z x4 dx + λ vu dx = v(x4) (x4) − v(x0) (x0) − vf dx. x0 dx dx x0 dx dx x0
Therefore, using Eq. (2.3) along with the fact that v is zero at x = x0, one obtains
Z x4 dv du Z x4 Z x4 dx + λ vu dx = v(x4)gN − vf dx. (2.4) x0 dx dx x0 x0
Eq. (2.4) is a weak (or variational) form of Eq. (2.1). It should be noted that the Neumann boundary condition defined by Eq. (2.3) is naturally included within this weak formulation. Solutions to Eq. (2.4) are known as weak solutions to Eq. (2.1).
2.2.3 An Approximate Solution
Consider a generic approximation uδ = uδ(x) to the solution u. Further, consider writing this approximate solution as the sum of two components, namely uD and δ uH , such that
δ δ u = uD + uH , (2.5)
where uD is a known function that satisfies the Dirichlet boundary condition at δ x = x0, and uH is an unknown function (to be determined) that is zero on the
Dirichlet boundary at x = x0. Note that the superscript δ is omitted from uD since δ uD is a known function, not an approximation. The approximate nature of u is δ contained within uH . Also note that due to this decomposition, the approximate δ solution u will always satisfy the Dirichlet boundary condition at x = x0 exactly.
If u is replaced by uδ in Eq. (2.4) (and also if v is replaced with a generic approxima- tion vδ which is exactly zero on Dirichlet boundaries) then the following expression
45 is obtained
Z x4 δ δ Z x4 Z x4 dv du δ δ δ δ dx + λ v u dx = v (x4)gN − v f dx. (2.6) x0 dx dx x0 x0
Substitution of Eq. (2.5) into Eq. (2.6) leads to
Z x4 δ δ Z x4 dv duD duH δ δ + dx + λ v (uD + uH ) dx = x0 dx dx dx x0
Z x4 δ δ v (x4)gN − v f dx, x0 and hence
Z x4 δ δ Z x4 dv duH δ δ dx + λ v uH dx = x0 dx dx x0
Z x4 Z x4 δ Z x4 δ δ dv duD δ v (x4)gN − v f dx − dx, −λ v uD dx. (2.7) x0 x0 dx dx x0
The problem as formulated by Eq. (2.7) includes all boundary conditions. Note that all terms on the right hand side of Eq. (2.7) are either known or arbitrary.
2.2.4 A Spectral/hp Element Basis
δ δ The approximations uH and v are as yet undefined. In order to proceed with a description of the spectral/hp element method, it is necessary to cast these approx- imations in terms of a global spectral/hp basis. There are two important steps in the formation of a spectral/hp basis. The first is to partition the solution domain into elements (an h-type discretisation). This step is often referred to as defining a mesh on the domain. The second step is to define a spectral basis locally within each element of the domain (a p-type discretisation). The mesh, along with the spectral basis within each element, can then be used to define a global spectral/hp basis within the entire domain.
46 Consider constructing a mesh on the domain Ω. In this example Ω will be split into four non-overlapping elements defined as
Ω0 = {x | x0 ≤ x ≤ x1}, Ω1 = {x | x1 ≤ x ≤ x2},
Ω2 = {x | x2 ≤ x ≤ x3}, Ω3 = {x | x3 ≤ x ≤ x4}, where
x0 < x1 < x2 < x3 < x4, and hence
3 3 [ \ Ω = Ωi Ωi = ∅. i=0 i=0
Further to this definition of a mesh, consider constructing a spectral basis within each element Ωi. To facilitate such a process it is useful to introduce the concept of a standard element ΩS = {ρ | − 1 ≤ ρ ≤ 1}. For each element Ωi bounded between xi and xi+1 (where i = 0, 1, 2, 3), a mapping Si between ρ within ΩS and x within Ω can be defined as
1 − ρ 1 + ρ x = S (ρ) = x + x ρ ∈ Ω . i 2 i 2 i+1 S
Hence, for each element Ωi bounded between xi and xi+1 (where i = 0, 1, 2, 3), an −1 inverse mapping Si between x within Ω and ρ within ΩS can also be defined as
−1 x − xi ρ = Si (x) = 2 − 1 x ∈ Ωi. xi+1 − xi
rd S S Within the standard element ΩS a 3 order modal polynomial basis φj = φj (ρ), containing four modes, can be defined as 1 − ρ j = 0 2 1 − ρ1 + ρ S 1,1 φj = P (ρ) 0 < j < 3 (2.8) 2 2 j−1 1 + ρ j = 3, 2
47 1,1 where Pj−1(ρ) are Jacobi polynomials. Note that a variety of spectral bases could have been used within the standard element. Other types of basis will be discussed shortly in Section 2.2.9.
S The basis φj within the standard element ΩS, along with the mappings between ΩS and each element Ωi of Ω, can be used to define a global spectral/hp basis within Ω. Here it will be required that the global basis is C0 continuous i.e. it will be required that the global basis functions are continuous everywhere (but the first and further derivatives of the functions need not be). With this constraint in mind, a global spectral/hp basis Φk = Φk(x) within Ω can be defined as
S −1 S −1 φ0 (S0 (x)) x ∈ Ω0 φ1 (S0 (x)) x ∈ Ω0 Φ0(x) = Φ1(x) = 0 x∈ / Ω0 0 x∈ / Ω0
S −1 φ3 (S0 (x)) x ∈ Ω0 S −1 φ2 (S0 (x)) x ∈ Ω0 Φ (x) = Φ (x) = S −1 2 3 φ0 (S1 (x)) x ∈ Ω1 0 x∈ / Ω 0 0 x∈ / Ω0 ∪ Ω1
S −1 S −1 φ1 (S1 (x)) x ∈ Ω1 φ2 (S1 (x)) x ∈ Ω1 Φ4(x) = Φ5(x) = 0 x∈ / Ω1 0 x∈ / Ω1
S −1 φ3 (S1 (x)) x ∈ Ω1 S −1 φ1 (S2 (x)) x ∈ Ω2 Φ (x) = S −1 Φ (x) = 6 φ0 (S2 (x)) x ∈ Ω2 7 0 x∈ / Ω 2 0 x∈ / Ω1 ∪ Ω2
48 S −1 φ3 (S2 (x)) x ∈ Ω2 S −1 φ2 (S2 (x)) x ∈ Ω2 Φ (x) = Φ (x) = S −1 8 9 φ0 (S3 (x)) x ∈ Ω3 0 x∈ / Ω 2 0 x∈ / Ω2 ∪ Ω3
S −1 S −1 φ1 (S3 (x)) x ∈ Ω3 φ2 (S3 (x)) x ∈ Ω3 Φ10(x) = Φ11(x) = 0 x∈ / Ω3 0 x∈ / Ω3
S −1 φ3 (S3 (x)) x ∈ Ω3 Φ12(x) = 0 x∈ / Ω3
Since the global basis Φk is constructed from a mesh containing four elements, and each element is spectrally decomposed into four modes, one may expect the basis to be formed of 16 = 4 × 4 global modes. However, due to the requirement of C0 continuity at the three inter-element interfaces there are three constraints, and hence only 13 = (4 × 4) − 3 global modes in the basis. It can be noted that only five of the 13 modes have values at elemental boundaries, these modes are known as global boundary modes. The remaining modes, which are zero at elemental boundaries, are known as global interior modes. The basis functions Φk are illustrated graphically in Fig. 2.1.
49 1 1 1
0.8 0.8 0.8
0.6 0.6 0.6
0 0.4 1 0.4 2 0.4 ! ! !
0.2 0.2 0.2
0 0 0
-0.2 -0.2 -0.2 x x x x x x x x x x x x x x x 0 1 x2 3 4 0 1 x2 3 4 0 1 x2 3 4
1 1 1
0.8 0.8 0.8
0.6 0.6 0.6
3 0.4 4 0.4 5 0.4 ! ! !
0.2 0.2 0.2
0 0 0
-0.2 -0.2 -0.2 x x x x x x x x x x x x x x x 0 1 x2 3 4 0 1 x2 3 4 0 1 x2 3 4
1 1 1
0.8 0.8 0.8
0.6 0.6 0.6
6 0.4 7 0.4 8 0.4 ! ! !
0.2 0.2 0.2
0 0 0
-0.2 -0.2 -0.2 x x x x x x x x x x x x x x x 0 1 x2 3 4 0 1 x2 3 4 0 1 x2 3 4
1 1 1
0.8 0.8 0.8
0.6 0.6 0.6 0 1 9 0.4 1 0.4 1 0.4 ! ! ! 0.2 0.2 0.2
0 0 0
-0.2 -0.2 -0.2 x x x x x x x x x x x x x x x 0 1 x2 3 4 0 1 x2 3 4 0 1 x2 3 4
1
0.8
0.6 2
1 0.4 ! 0.2
0
-0.2 x x x x x 0 1 x2 3 4
Figure 2.1: Graphical illustration of global spectral/hp basis functions Φk. 50 2.2.5 Galerkin Approximation
δ δ δ It is now possible to represent u = uD +uH and v in terms of the global spectral/hp basis Φk. Here it will be chosen that
uD = gDΦ0, (2.9)
12 δ X uH = uˆkΦk, (2.10) k=1
12 δ X v = vˆlΦl, (2.11) l=1
δ whereu ˆk are coefficients to be determined, andv ˆl are arbitrary coefficients since v is arbitrary. It can be noted that uD is written in terms of the known function Φ0, since this is the only basis function which is non-zero on the Dirichlet boundary at
δ δ x = x0. It can also be noted that uH and v are both represented by the same basis functions, all of which are zero on Dirichlet boundaries. A implementation such as
δ δ this, where identical bases are used to represent both uH and v , is often referred to as a Galerkin type implementation.
2.2.6 Global Matrix Equation
On substituting Eq. (2.9), Eq. (2.10) and Eq. (2.11) into Eq. (2.7), one obtains
12 12 12 12 Z x4 Z x4 X X dΦk dΦl X X uˆ vˆ dx + λ uˆ vˆ Φ Φ dx = k l dx dx k l k l k=1 l=1 x0 k=1 l=1 x0
12 12 Z x4 Z x4 X X dΦl dΦ0 vˆ g − vˆ Φ f dx − vˆ g dx− 12 N l l l D dx dx l=1 x0 l=1 x0
12 X Z x4 λ vˆlgD ΦlΦ0 dx. (2.12) l=1 x0
51 Defining the matrices
Z x4 Z x4 dΦk dΦl L[k][l] = dx, M[k][l] = ΦkΦl dx, x0 dx dx x0 and the vectors
uˆ[k] =u ˆk, vˆ[l] =v ˆl,
0 l 6= 12 Z x4 n[l] = , f[l] = Φlf dx, x0 gN l = 12
Z x4 Z x4 dΦl dΦ0 d[l] = gD dx − λ ΦlΦ0 dx , x0 dx dx x0 where L[1][1] and M[1][1] denote the top left entries in L and M respectively, and uˆ[1][1], vˆ[1][1], n[1], f[1] and d[1] denote the first entries in uˆ, vˆ, n, f and d respec- tively, one can write Eq. (2.12) succinctly in matrix form as
vˆ>(L + λM)uˆ = vˆ>(n − f − d). (2.13)
Since vδ is arbitrary, vˆ is also arbitrary, and thus Eq. (2.13) is only satisfied if
(L + λM)uˆ = (n − f − d). (2.14)
On pre-multiplication of Eq. (2.14) by (L + λM)−1 one obtains the following ex- pression for uˆ (and hence the approximate weak solution uδ)
uˆ = (L + λM)−1(n − f − d). (2.15)
2.2.7 Matrix Structure
The matrix L is often referred to as the global Laplacian matrix of the system, and the matrix M is often referred to as the global mass matrix of the system. It can be
52 noted that both L and M have some degree of structure. Implementations of the spectral/hp element method seek to use such structure in order to facilitate matrix creation, storage and inversion.
The structure of the global mass matrix M can be illustrated in the following schematic fashion
∗ 0 0 0 0 0 0 0 0 0 ∗ 0 0 0 0 0 0 0 0 0 ∗ ∗ N ∗ ∗ N 0 0 0 0 0 0 0 0 ∗ ∗ 0 0 0 0 0 0 0 0 ∗ ∗ 0 0 0 0 0 0 0 0 N ∗ ∗ N ∗ ∗ N 0 0 0 M = , 0 0 0 0 0 ∗ ∗ 0 0 0 0 0 0 0 0 ∗ ∗ 0 0 0 0 0 0 0 0 N ∗ ∗ N ∗ ∗ N 0 0 0 0 0 0 0 0 ∗ ∗ 0 0 0 0 0 0 0 0 ∗ ∗ 0 0 0 0 0 0 0 0 N ∗ ∗ N where the solid black triangles represent non-zero entries due to coupling between global boundary modes, the asterisks represent non-zero entries due to coupling between global boundary modes and global interior modes, and the solid black squares represent non-zero entries due to coupling between global interior modes. It can be noted that M is symmetric due to the form of the Helmholtz operator in Eq. (2.1) and the nature of the weak form derived in Eq. (2.4). Also, many of the entries in M are zero due to orthogonality between various global modes.
Additional structure of M is revealed if entries within the solution vector uˆ and the right hand side vectors n, f and d are re-ordered. Specifically, consider defining a re-ordering matrix R as
53 001000000000 000001000000 000000001000 000000000001 100000000000 010000000000 R = . 000100000000 000010000000 000000100000 000000010000 000000000100 000000000010
On multiplication of uˆ, n, f and d by R one obtains the vectors uˆR = Ruˆ, nR = Rn, fR = Rf and dR = Rd, which are all ordered such that global boundary modes appear first, followed by global interior modes. Eq. (2.15) can be rewritten in terms of uˆR, nR, fR and dR as
−1 uˆR = (LR + λMR) (nR − fR − dR), (2.16) where
−1 −1 LR = RLR , MR = RMR .
Eq. (2.16) encodes the same information as Eq. (2.15). However, entries within LR and MR are rearranged c.f. entries in L and M respectively. Specifically, MR has the modified form
54 NN 0 0 ∗ ∗ ∗ ∗ 0 0 0 0 NNN 0 0 0 ∗ ∗ ∗ ∗ 0 0 0 NNN 0 0 0 0 ∗ ∗ ∗ ∗ 0 0 NN 0 0 0 0 0 0 ∗ ∗ ∗ 0 0 0 0 0 0 0 0 0 ∗ 0 0 0 0 0 0 0 0 0 MR = ∗ ∗ 0 0 0 0 0 0 0 0 ∗ ∗ 0 0 0 0 0 0 0 0 0 ∗ ∗ 0 0 0 0 0 0 0 0 ∗ ∗ 0 0 0 0 0 0 0 0 0 ∗ ∗ 0 0 0 0 0 0 0 0 ∗ ∗ 0 0 0 0 0 0 where the solid black triangles, asterisks, and solid black squares represent various non-zero entries as previously described.
The structure of MR is apparent, with boundary-boundary interactions grouped in the top left quadrant, boundary-interior interactions grouped in the top right and bottom left quadrants, and interior-interior interactions grouped in block diagonal form in the bottom right quadrant. The structure of MR lends its self to inversion via a static condensation method, which avoids explicit construction, storage and inversion of the entire matrix. For further details see Karniadakis and Sherwin [59].
2.2.8 Global Assembly
Due to the elemental structure of a spectral/hp element basis, it is possible to assemble global matrices (such as M) and global vectors (such as d) from their elemental contributions. The ability to assemble global matrices and global vectors from elemental contributions is advantageous for several reasons. In particular, it allows operations such as integration to be carried out solely at an elemental level
55 within a standard element, rather than throughout the entire domain.
To illustrate the procedure of global matrix assembly consider defining a matrix m as
m0 0 0 0 0 m1 0 0 m = , 0 0 m2 0 0 0 0 m3 where
Z 1 S S dSi mi[n][m] = φn−1(ρ)φm−1(ρ) dρ (i = 0, 1, 2, 3), −1 dρ
with each mi[1][1] denoting the top left entry of each elemental mass matrix mi. The global mass matrix M can be assembled from the elemental mass matrices held within m via the following matrix manipulation
M = A>mA, where A is an assembly matrix defined as
56 000000000000 100000000000 010000000000 001000000000 001000000000 000100000000 000010000000 000001000000 A = . 000001000000 000000100000 000000010000 000000001000 000000001000 000000000100 000000000010 000000000001
It can be noted that columns three, six and nine of the assembly matrix A contain two non-zero entries (whereas all other columns contain only one). This is because the global modes Φ3,Φ6 and Φ9 are constructed from two local modes, whereas all other global modes are constructed from only one. Also, it can be noted that the top row of A contains all zero entries. This is because none of the global modes
δ S used in the expansion of uH contain the local mode φ0 mapped to the element Ω0. Finally, it can be noted that A is rectangular, not square, since there are more local degrees of freedom than global degrees of freedom.
In practice (since A is very sparse) M is not assembled via matrix manipulations; instead it is assembled using a series of mappings. For further details of the afore- mentioned global matrix assembly procedure see Karniadakis and Sherwin [59].
57 2.2.9 Other Elemental Bases
The elemental basis defined by Eq. (2.8) is an example of a modal basis. Modal bases are heirarchical in nature, that is to say lower order modal expansions are subsets of higher order modal expansions. Other types of expansion basis can also be used to represent the solution within a standard element, including those that are nodal in nature (which are defined in terms of a set of nodal points situated within the standard element). Such nodal bases are not heirarchical in nature, that is to say higher order nodal expansions cannot be formed by adding further modes to lower order nodal expansions.
When choosing an appropriate elemental basis one should take several factors into consideration. In particular it is preferable that the basis functions are orthogonal (or at least near to being orthogonal), so as to reduce coupling between elemental modes. Also, it is preferable that the basis can be decomposed into boundary and interior modes, since this facilitates the enforcement of C0 continuity between adjacent elements. Other considerations include how linearly independent the basis functions are, since this will impact the conditioning of any matrices that are formed (which in turn affects the ease with which matrices can be numerically inverted). For further details regarding the choice of suitable basis functions see Karniadakis and Sherwin [59].
2.3 Extension to Two-Dimensions
2.3.1 Overview
The basic principles of the spectral/hp element method previously described within a 1D context also apply in multiple dimensions. It is the case, however, that extension of the method to multiple dimensions gives rise to several additional complications. The most notable of these complications is the fact that a standard element (which is simply a line segment in 1D) can take various forms in multiple dimensions. In
58 2D, standard elements can take the form of quadrangles or triangles. An overview of suitable basis functions within such quadrangular and triangular standard elements is given below.
2.3.2 Basis Functions Within Quadrangular Elements
A quadrangular standard element ΩSQ is illustrated in Fig. 2.2, and can be defined mathematically in the following fashion
ΩSQ = (ρ1, ρ2 | − 1 ≤ ρ1 ≤ 1, −1 ≤ ρ2 ≤ 1).