Rad 226A/Bioe 226A Winter 2018-2019 in Vivo MR: Spin Physics and Spectroscopy

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Rad 226A/Bioe 226A Winter 2018-2019 in Vivo MR: Spin Physics and Spectroscopy Rad 226a/BioE 226a Winter 2018-2019 In Vivo MR: Spin Physics and Spectroscopy Daniel Spielman, Ph.D., Dept. of Radiology ! Lucas Center for MR Spectroscopy and Imaging! (corner of Welch Rd and Pasteur Dr)! office: Lucas Center PS-061, phone: x3-8697 email: [email protected]! 1 Limitations of Non-interacting Classical Model • Relaxation – Tissue T1, T2, and T1ρ – Anisotropic tissues • Nuclei other than 1H • Chemical exchange effects • Molecules more complicated than water Does it matter that water has two 1H nuclei? O H H 2 Image Contrast • Clinical MRI primarily images water. Why do different tissues exhibit different MRI contrast? Are difference solely due to water content? Proton Density T1 T2 T1ρ map Post-GD T1 CEST SWI 3 Lecture #1! Introduction • Topics – Administrative details – Course Overview and Motivation – Some interesting in vivo MR phenomena • Handouts and Reading Assignments – Biographies: Rabi, Purcell, Bloch 4 Course Administration • Lectures – Tues, Thurs 3:00-4:20 pm, Lucas Learning Center P-069 – 3 units • TA – ?? • Office Hours – To be determined, Office: Lucas Center PS061 – or by arrangement with instructor (email: [email protected]) • Web site – http://web.stanford.edu/class/rad226a/ – Lecture notes, homework assignments, other handouts (pdf files) 5 Course Materials • Recommended Texts – F. van de Ven, Multidimensional NMR in Liquids, Wiley- VCH, New York, 1995. – R. de Graaf, In Vivo NMR Spectroscopy, 2nd Edition, Wiley & Sons, Chichester, UK, 2007 • Additional references (not required, but very useful!) MRI • D. Nishimura, Principles of Magnetic Resonance Imaging, EE369b notes Physics • M. Levitt, Spin Dynamics, Wiley, Chichester. UK, 2001 QM • D. Miller, Quantum Mechanics for Scientists and Engineers, Cambridge Univ. Press, 2008. Physics • C. Slichter, Principles of Magnetic Resonance, Springer, Berlin, 1996. 6 Assignments and Grading • Weekly problem sets (90%) • Class participation (10%) • No Midterm or Final 7 Overview • Main Themes: – Classical vector model of MRI/MRS doesn’t fully explain many important in vivo processes, particularly those involving interactions among spins. – Nuclear-nuclear interactions – Nuclear-electron interactions – We’ll discuss the physics and engineering principles of these phenomena with examples from current research topics and clinical applications. • Prerequisites – EE369b or familiarity with MRI (i.e. Rf pulses, gradients, pulse sequence diagrams, k-space) – Working knowledge of linear algebra 8 Roadmap POF Density Matrix Double quantum coherence? Quantum J-coupling? Mechanics PolarizationPolarization and Math transfer?transfer? MR Physics MRPhysics Bloch equations, k-space, selective excitation, … (EE369b) large break (prerequisites) Intuition Have you tried using the full density matrix? Topics 1. Introduction and Review (2 weeks) 5. 1H MRS (1.5 weeks) 2. Quantum mechanics for NMR (2 week) 6. Decoupling (stealth lead-in to relaxation theory) (1 week) 3. Density Matrix (1 week) 4. Product Operator Formulism (1.5 weeks) 9 Spectroscopy • In general, spectroscopy is the study of materials via interactions with electromagnetic fields EM radiation Spectroscopy NMR and Molecular Spies 1022 γ-rays While molecules are too small to observe 1020 Mössbauer x-rays energy of directly, magnetic nuclei make ideal probes: 18 chemical bonds 10 • Very sensitive to the local magnetic fields ultraviolet 1016 electronic • Interact extremely weakly with their visible 1014 environment permitting virtually infrared vibrational thermal 1012 energy @37C perturbation-free measurements microwave 1010 rotational • Spatially localized 108 NMR RF Note: These differ by several orders of magnitude! 106 Hz Energy 10 NMR: A Short History Discovery of NMR NMR in Condensed Matter r1937 1945 ˆ B = B0z µ z r θ µ θ = 54.7!, I = 1 , m = 1 2 2 1 " 3 µ = γ , µ = γ z 2 ! 2 ! E. Purcell € I.I. Rabi F. Bloch € Nobel Prize Physics Nobel Prize Physics 1952 1944 11 NMR: A Short History Determining 3D structures of FT-NMR, 2D Spectroscopy biological macromolecules 1966-1970s 1980s 1D Spectrum 2D Spectrum 3D Spectrum R. Ernst K. Wüthrich Nobel Prize Chemistry Nobel Prize Chemistry 12 1991 2002 NMR in the Chemistry Laboratory • Types of NMR spectroscopy experiments most relevant for – High resolution studies of liquids in vivo studies – Solid state NMR (e.g. magic angle spinning) – Studies of substances (or nuclei) with broad resonance lines • Types of Questions – What is it? – What is the structure? bonding connectivity spatial connectivity molecular conformation – What are the dynamics? 13 In Vivo MRS/MRI pure liquid tissue crystalline solid • Complex mixture of stuff – P. Lauterbur P. Mansfield water, lipids, metabolites, etc • Physiological processes • Types of Questions – Where is it? Nobel Prize: Medicine 2003 – How much? – What are the dynamics? relaxation times chemical processes 14 MRI • Standard analysis based on a water signal made up of many independent (non-interacting) nuclei + phenomenological T1 and T2 relaxation times. • Leads to very powerful approaches (e.g. k-space) that adequately explain the bulk of MRI techniques and applications. 15 Limitations of Non-interacting Classical Model • Relaxation – Tissue T1, T2, and T1ρ – Anisotropic tissues • Nuclei other than 1H • Chemical exchange effects • Molecules more complicated than water Does it matter that water has two 1H nuclei? O H H 16 Example: Temperature effects Hydrogen NMR Spectrum bonds Liquid water peak water T effects? ppm 1 Which is the correct model for the effect of temperature? “Chemical shift “T model” “Two-pools model” 2 model” T= 37º C T = 38º C T = 39º C T= 39º C T= 39º C Protons w/o T = 38º C hydrogen T = 38º C bonds T = 37º C Protons w/ hydrogen T = 37º C bonds ppm ppm ppm ppm ppm 17 Example: Water, water, water 2 • Consider a mixture with 5% D2O and 95% H2O (D = H) O O O 1 1 1 1 O O H H H H 1 1 1 1 O H H H H 1 1 O O H H 2H 1H 1 1 2H 1H H H O O O 1 2 O 1 1 O H H 1 1 H H 2 2 H H 1H 1H H H Why is T1, D << T1, H? What about T2, D vs T2, H? What if the solution in injected in vivo? 17 16 • Consider a mixture with 5% H2 O and 95% H2 O 17 16O 16 16 O 16O O O 16O H H 16 H H 16O 16O H H H H 17O H H H H O H H H H H H H H 16 Why is the proton T2 for this mixture < T2 for a pure H2 O sample? What about T ? 1 18 Example: Tendon Imaging • T2 of tendons is strongly dependent on the angular o orientation with respect to B0: magic angle = 54.7 o Tendon parallel to B0 Tendon angle = 55 B0 B0 acute Achilles tendon rupture: 3D GRE, TR/TE=21/7 ms What about T1? 19 Example: Fast Spin Echo T2 • Why is fat bright on FSE images? Conventional Spin Echo Fast Spin Echo TR/TE=2500/80 ms TR/TE=2500/80 ms, ETL = 8 20 Example: γ-aminobutyric acid (GABA) x 300 How? • Why? GABA 1H Brain Spectrum (with suppression of everything GABA/glutamate are the major except GABA) excitatory/inhibitory GABA neurotransmitters in the human brain, and are of particular interest for conditions such as autism, for ? ? ? which an excitatory/inhibitory x 3000 imbalance is hypothesized. 21 Example: Brain tumors 52 y.o male: MRI #1 - rule out stroke, MRI #2 - tumor? choline choline NAA creatine creatine NAA TE = 144 ms TE = 144 ms post-contrast T1 9 y.o male: non-enhancing lesion in left hippocampus NAA choline choline creatine creatine NAA TE = 144 ms TE = 144 ms 22 post-contrast T1 Next lecture: ! Review of Classical MR 23 Biography: Isidor Isaac Rabi (born July 29, 1898, Rymanów, Austria-Hungary [now in Poland]—died Jan. 11, l988, New York, N.Y., U.S.) American physicist who was awarded the Nobel Prize for Physics in 1944 for his invention (in 1937) of the atomic and molecular beam magnetic resonance method of observing atomic spectra. Rabi's parents settled in New York City in 1899. After earning a bachelor's degree in chemistry at Cornell University in 1919, Rabi switched to physics and received his Ph.D. from Columbia University in 1927. He did postgraduate work in Europe and then joined the faculty of Columbia University in 1929, becoming professor of physics in 1937. From 1940 to 1945 Rabi was a leader of the group of scientists at the Massachusetts Institute of Technology, Cambridge, who helped in the development of radar. He was a member of the General Advisory Committee of the Atomic Energy Commission from 1946 to 1956 and succeeded J. Robert Oppenheimer as its chairman from 1952 to 1956. He originated the concept of the CERN international laboratory for high-energy physics in Geneva, Switz., and he was one of the founders of the Brookhaven National Laboratory, Upton, N.Y. He also built up one of the world's finest physics departments at Columbia University, one which was to produce several Nobel Prize–winning physicists. Rabi's most important scientific work was his development (in the 1930s) of a method for measuring the magnetic properties of atoms, atomic nuclei, and molecules. The method is based on measuring the spin of the protons in the atom's core, a phenomenon known as nuclear magnetic moments. With the application of his magnetic resonance method, several mechanical and magnetic properties, as well as the shape, of an atomic nucleus can be deduced. The precise measurements yielded by this method made possible such subsequent applications as the atomic clock, the maser, and the laser, as well as the nuclear magnetic resonance imaging used in diagnostic medicine. Rabi's method provided the central technique for virtually all molecular and atomic beam experimentation.
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