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Cosmological post-Newtonian Approximation compared with
Perturbation Theory
J. HwangKNU/KIAS2012.02.17
Question
Compared with Einstein’s gravity, is Newton's gravity reliable in near horizon scale simulation?
Linear deviation from homogeneous-isotropic background
Action at a distance
Newton’s theory: Non-relativistic (no c)
Action at a distance, violate causality c=∞ limit of Einstein’s gravity: 0th post-
Newtonian limit No horizon Static nature
No strong pressure No strong gravity No gravitational waves Incomplete and inconsistent
Einstein’s gravity: Relativistic Strong gravity, dynamic Simplest
Perturbation method: Perturbation expansion All perturbation variables are small Weakly nonlinear Strong gravity; fully relativistic Valid in all scales
Post-Newtonian method: Abandon geometric spirit of GR: recover the
good old absolute space and absolute time Provide GR correction terms in the Newtonian
equations of motion Expansion in strength of gravity
Fully nonlinear No strong gravity situation; weakly relativistic Valid far inside horizon
FullyRelativistic
FullyNonlinear
WeaklyRelativistic
WeaklyNonlinear
?
Studies of Large-scale Structure
NewtonianGravity axis
Linear Perturbation
Background World Model axis
FullyRelativistic
FullyNonlinear
WeaklyRelativistic
Post-Newtonian (PN)Approximation
Pert
urb
ati
on
Th
eory
(P
T)
“Terra Incognita”Numerical Relativity
PT vs. PN
WeaklyNonlinear
NewtonianGravity axis
Background World Model axis
FullyRelativistic
FullyNonlinear
WeaklyRelativistic
“Terra Incognita”Numerical Relativity
Cosmological 1st order Post-Newtonian (1PN)
Cosmological Nonlinear Perturbation (2nd and 3rd order)
Linear Perturbation vs. 1PN
WeaklyNonlinear
NewtonianGravity axis
Linear Perturbation
Background World Model axis
Mass conservation:
Momentum conservation:
Poisson’s equation:
Newtonian perturbation equations:
Newtonian (0PN) metric:
Metric convention: (Bardeen 1988)
Spatial gauge:
Bardeen, J.M. in “Particle Physics and Cosmology” edited by Fang, L., & Zee, A. (Gordon and Breach, London, 1988) p1
Relativistic/Newtonian correspondences:
Comoving gauge Zero-shear gauge
Uniform-expansion-gauge Uniform-curvature gauge
Perturbed density, Perturbed velocity
Perturbed gravitational potential Perturbed curvature
JH, Noh, Gong (2012)
Relativistic/Newtonian correspondence includes Λ, but assumes:
1. Flat Friedmann background2. Zero-pressure3. Irrotational4. Single component fluid5. No gravitational waves6. Second order in perturbations
Relaxing any of these assumptions could lead to pure general relativistic effects!
Linear order: Lifshitz (1946)/Bonnor(1957)
Second order: Peebles (1980)/Noh-JH (2004)
Third order: JH-Noh (2005)
Physical Review D 69 10411 (2004); 72 044012 (2005)Pure General Relativistic corrections
(comoving-synchronous gauge)
Curvature perturbation in the comoving gauge
~10-5
(K=0, comoving gauge)
Jeong, Gong, Noh, JH, ApJ 722, 1(2011)
The unreasonable effectiveness of Newtonian gravity in cosmology!
Vishniac MN 1983
Jeong et al 2011
Pure Einstein
Minkowski background
Robertson-Walker background
Newtonian gravitational potential
JH, Noh, Puetzfeld, JCAP 03 010 (2008)
Zero-pressure 1PN equations:
Nonlinear
E-conservation:
Mom-conservation:
Raychaudhury-eq:G0
0-Gii
Mom-constraint:G0
i