C.D.S. - SIMBAD4 rel 1.7 - 2020.02.27CET17:15:43

2014A&A...562L...2C - Astronomy and Astrophysics, volume 562, L2-2 (2014/2-1)

Probing photon decay with the Sunyaev-Zel'dovich effect.


Abstract (from CDS):

The fundamental properties of the photon have a deep impact on the astrophysical processes that involve it, such as the inverse Compton scattering of CMB photon by energetic electrons residing within galaxy cluster atmospheres. This is usually referred to as the Sunyaev-Zel'dovich effect (SZE). We calculate the combined constraints on the photon decay time and mass by studying the impact of the modified CMB spectrum on the SZE of galaxy clusters. We analyze the modifications of the SZE as produced by photon decay effects. We study the frequency ranges where these modifications are large and where the constraints derived from the SZE are stronger than those already obtained from the CMB spectrum. We show that the SZE can set limits on the photon decay time and mass, or on E*=(t0)/(τγ)mγc2, which are stronger than those obtained from the CMB. The main constraints come from the low-frequency range ν≃10-50 GHz where the modified SZE ΔImod is greater than the standard one ΔI, with the difference |(ΔImod-ΔI)| increasing with the frequency for increasing values of E*. Additional constraints can be set in the range 120-180GHz where there is an increase in the frequency position of the minimum of ΔImod with respect to the standard one with increasing values of E*. We demonstrated that the effect of photon decay can be measured or constrained by the Square Kilometer Array in the optimal range ≃10-30GHz setting limits of E*≲1.4x10–9eV and 5x10–10eV for 30- and 260-h integration for A2163, respectively. These limits are tighter than those obtained with the COBE-FIRAS spectral measurements of the CMB.

Abstract Copyright:

Journal keyword(s): cosmology: theory - cosmic background radiation - galaxies: clusters: general

Simbad objects: 2

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Number of rows : 2

N Identifier Otype ICRS (J2000)
ICRS (J2000)
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
1 ClG 0657-56 ClG 06 58 29.6 -55 56 39           ~ 785 1
2 ACO 2163 ClG 16 15 34.1 -06 07 26           ~ 514 0

    Equat.    Gal    SGal    Ecl

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