Are we living near the center of a local void?

Autor: Giulia Cusin, Jean-Philippe Uzan, Cyril Pitrou
Přispěvatelé: Institut Lagrange de Paris, Sorbonne Universités, Institut d'Astrophysique de Paris ( IAP ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Sorbonne Université (SU)
Jazyk: angličtina
Rok vydání: 2017
Předmět:
High Energy Physics - Theory
Void (astronomy)
velocity
Cosmology and Nongalactic Astrophysics (astro-ph.CO)
polarization: anisotropy
[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]
Diagonal
Cosmic microwave background
Cosmic background radiation
FOS: Physical sciences
General Relativity and Quantum Cosmology (gr-qc)
Astrophysics::Cosmology and Extragalactic Astrophysics
cosmic background radiation
Correlation function (quantum field theory)
local void
01 natural sciences
General Relativity and Quantum Cosmology
[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]
[ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]
0103 physical sciences
effect: geometrical
structure
correlation function
symmetry: rotation
Anisotropy
010303 astronomy & astrophysics
Physics
[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]
010308 nuclear & particles physics
angular correlation
formation
anisotropy: measured
Astronomy and Astrophysics
Local Void
High Energy Physics - Theory (hep-th)
kinematics
Excited state
Quantum electrodynamics
[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]
polarization: correlation
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
signature
Astrophysics - Cosmology and Nongalactic Astrophysics
Zdroj: JCAP
JCAP, 2017, 03 (03), pp.038. 〈10.1088/1475-7516/2017/03/038〉
JCAP, 2017, 03, pp.038. ⟨10.1088/1475-7516/2017/03/038⟩
DOI: 10.1088/1475-7516/2017/03/038〉
Popis: The properties of the cosmic microwave background (CMB) temperature and polarisation anisotropies measured by a static, off-centered observer located in a local spherically symmetric void, are described. In particular in this paper we compute, together with the standard 2- point angular correlation functions, the off-diagonal correlators, which are no more vanishing by symmetry. While the energy shift induced by the off-centered position of the observer can be suppressed by a proper choice of the observer velocity, a lensing-like effect on the CMB emission point remains. This latter effect is genuinely geometrical (e.g. non-degenerate with a boost) and reflects in the structure of the off-diagonal correlators. At lowest order in this effect, the temperature and polarisation correlation matrices have non-vanishing diagonal elements, as usual, and all the off-diagonal terms are excited. This particular signature of a local void model allows one, in principle, to disentangle geometrical effects from local kinematical ones in CMB observations.
Comment: 49 pages, 8 figures
Databáze: OpenAIRE