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How to Cite Complete Issue More Information About This Article Scientia Et Technica ISSN: 0122-1701 [email protected] Universidad Tecnológica de Pereira Colombia Vija Suarez, Oscar Javier Characterization of the radiation and matter transfer functions Scientia Et Technica, vol. 23, no. 3, 2018, June-September, pp. 381-385 Universidad Tecnológica de Pereira Colombia Available in: https://www.redalyc.org/articulo.oa?id=84959041010 How to cite Complete issue Scientific Information System Redalyc More information about this article Network of Scientific Journals from Latin America and the Caribbean, Spain and Journal's webpage in redalyc.org Portugal Project academic non-profit, developed under the open access initiative Scientia et Technica Año XXIII, Vol. 23, No. 03, septiembre de 2018. Universidad Tecnológica de Pereira. ISSN 0122-1701 381 Characterization of the radiation and matter transfer functions Characterization of the radiation and matter transfer functions Oscar Javier Vija Suarez Observatorio Astronómico Nacional, Universidad Nacional, Bogotá D.C., Colombia [email protected] Abstract —This paper shows the characterization of the matter understand the perturbation evolution at matter epoch and and radiation transfer functions. The transfer functions provide how the perturbations grew up to become large structures. information about behavior of every species perturbation during radiation epoch, which allows to determine the evolution of these This paper shows the radiation and matter transfer function species during matter epoch. Graphics of the radiation and equations, related graphics and physical information about matter transfer functions, using the software CAMB are presented, in order to explain how large structures were formed. evolutions of perturbations. II. CONTENTS Key Word — Cosmological perturbations, Newtonian gauge, transfer function. To obtain and to study the radiation and matter transfer functions, it is necessary to start from the first model that I. INTRODUCTION explains the evolution of a homogenous and isotropic universe, also known as the background universe. Then, the The transfer function is a mathematical tool to explain a perturbations theory is presented, allowing to get a new model physical phenomenon in the period between inflation and to explain the dynamic of the perturbed universe, which is a Cosmic Microwave Background (CMB) [1]. It allows to better approximation to explain the current observations of the explain large galaxy clusters formation. The evolution of universe. Perturbation theory will be the methodology to find Universe is showed in the Figure 1. the equations of radiation and matter transfer functions. These functions will be graphed using the software CAMB and the physics that each of these involves will be discussed. A. The Background Universe Friedmann, Lemaitre, Robertson and Walker set a method to explain the Universe. This is a metric which describes a homogeneous, isotropic, expanding and flat universe [4,5]. It is called FLRW metric. Written in terms of conformal time ( τ) is: 2 2 2 i j ds= a(τ ) ( − d τ + δ ij dxdx ) , (1) Figure 1. Evolution of Universe. Taken from web site NASA [2] where a is the scale factor. Using FLRW metric, Einstein field equation can be solved. Einstein field equation is represented At bottom of Figure 1, the period of the transfer function as: explaining physical phenomena is shown. This period is called radiation epoch [3]. This paper focuses on this epoch, so, the Gµν=8π GT µν + g µν Λ , (2) solutions of the equations are presented in this period. where G is the Einstein tensor, which describes the universe The transfer function explains information transfer of the µν geometry. G is the gravitational constant; T is the Stress- perturbations behavior at radiation epoch, in order to µν Energy tensor. Regarding FLWR metric, Tµν corresponds a Fecha de Recepción: 30 de noviembre de 2017 Fecha de Aceptación: 20 de mayo de 2018 382 Scientia et Technica Año XXIII, Vol. 23, No. 03, septiembre de 2018. Universidad Tecnológica de Pereira. perfect fluid model. g is the metric tensor (FLRW), and Λ 2 2 2 i j µν dsa= −+12ψτ d ++ 12 φδ dxdx . (5) is the cosmological constant [5]. ( ( ) ( ) ij ) Friedman wanted to describe the universe dynamics. By Other perturbed magnitudes are defined. They are the density solving the equation (2) with the metric (1), Friedmann perturbation and the temperature [11,12] given by: equations are obtained [1,3,6]. These equations are: δρ δT δ = y θ = . (6) ρ T 2 2 a' 8 π G a Λ With equation (5), Einstein field equation (2) can be solved to =a2ρ + , (3) a 3 3 obtain: 2 ′ 2 2 a' a ' 2 2 kφ+3 H ψ ' + H φ =− 4 π Ga δρ (7) 2 + = 8 πGa P +Λ a . (4) ( ) a a a ' 22 2 2 From where can defined the Hubble parameter as H = , ψφ''2'+()HHH ++() 2'' ψφ +− k() φψπδ −= 4 GaP a 3 which refers to universe rate expansion, and the Hubble radius . (8) c which is the limit of causal interactions. It is R = , Other equation to be solved is the Boltzmann equation: H H where c is the light speed [5,7]. df = C , (9) B. The Perturbed Universe dt The universe described by FLRW couldn’t explain the new where f represents the distribution function for the species and observations of the universe, made with different probes. One C is the collision term [1,12]. This equation represents the of the observations was the Cosmic Microwave Background evolution of the distribution function of species, taking into (CMB), as shown in the Figure 2. The observations of account the interaction between them. inhomogeneities in the universe are presented. Because of, it was necessary to include the perturbations theory. In this investigation, the Boltzmann equation for photons and for dark matter is calculated. Dark matter is chosen because it is more abundant than baryonic matter [13]. The Boltzmann equation for photons is given by the equation: θ'+ik µθφ −+ ' ik µψ =− χθ '(0 −+ θµ v b ) , (10) where k is the wave number, which indicates that we are working in the Fourier space, θ is the perturbation in the temperature. μ is a parameter that indicates the direction of the photons. vb is the peculiar speed of the barons. θ0 it is the temperature monopole and χ is the optical depth, which Figure 2. CMB reported by missions COBE, WMAP and Planck . determines how opaque is the universe, at a determined time Taken from web site NASA [8] [12]. The perturbation theory proposes to represent the perturbed The Boltzmann equations for matter are: universe using the background universe. However, to make the identification between both, background and perturbed δ'+ikv cdm − 3'0 φ = , (11) universes, a gauge must be chosen [5,9,10]. For this research the Newtonian gauge is selected. It is because this gauge a ' explains the structures formation [9,11]. This gauge v'+ v + ik ψ = 0 . (12) cdma cdm introduces two perturbed potentials, ψ y ϕ, in the FLRW metric, obtaining a perturbed metric described by: Equation (11) determines the evolution of dark matter density, where v cdm is the peculiar velocity of dark matter [12]. Scientia et Technica Año XXIII, Vol. 23, No. 03, septiembre de 2018. Universidad Tecnológica de Pereira. 383 Equation (12) represents the evolution of the peculiar speed of scales the photons do not interact causally with other particles. dark matter. However, for sub-horizon scales, an oscillatory behavior is observed. This is due to the photons to interact with the With the equations (7), (8), (10), (11) and (12), the system of baryons for these scales, constituting the baryonic acoustic equations that describes the dynamics of the perturbed oscillations (BAO) phenomenon [12]. universe is complete. The solutions of the system equations are the radiation and matter transfer functions [12]. C. Radiation Transfer Function. In order to obtain the radiation transfer function, equation (10) is rewritten as: θ'+(ik µχθφ − '') =− ik µψχθ − ' ( 0 + iv µ b ) (13) This is a differential equation for the temperature perturbation θ [12,14]. The equation (13) is solved by line of sight method [15], which allows to express the solution in two functions: a geometric one, given by the spherical Bessel functions (j l) and other for interactions, S, known as the temperature sources function [12,15]. This sources function is compound by three effects known as the Sachs Wolfe effect, Doppler Effect and the Sachs Wolfe Integrated Effect [12]. The solution of it is the radiation transfer function and is given by: Figure 3. Radiation transfer function obtained with CAMB. This graphics represents the evolution of temperature perturbation with θτl(,)0k [ θτ l (,) 0 k+ ψτ ldec ( ,) kjk] l( ( ττ 0 − dec )) respect to the scales. −1 +kvb(τ dec ,)' kjk l( ( τ0 − τ dec )) τ0 This oscillating behavior also allows to deduce that matter and dτφτ'( , k )+ ψτ '( , kjk ) ττ − (14) radiation were grouped and separated, since the oscillations []l0 l dec l()()0 dec represent overdensities and subdensities [12]. The presence of τ dec overdensities imply that matter grouped, which later caused the large structures formation. In the first line of equation (14), the Sachs Wolfe effect is shown; this effect describes the temperature perturbation D. Matter Transfer Function. evolution and its interaction with the gravitational potential. In the second line the Doppler effect can be observed. This term Being interested to know matter perturbations evolution and describes how the peculiar speed of the barons affected the being able to know at what moment the large structures were distribution of the photons. Finally, line three belongs to the formed, we proceed to find the matter transfer function. integrated Sachs Wolfe effect, which is an integral that To find this function we start from equations (11) and (12). describes the evolution of the gravitational potentials from the Combining them we obtain the dark matter perturbations time of decoupling to our days.
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