CaltechAUTHORS
  A Caltech Library Service

Gamma-ray probe of cosmic ray pressure in galaxy clusters and cosmological implications

Ando, Shin'ichiro and Nagai, Daisuke (2008) Gamma-ray probe of cosmic ray pressure in galaxy clusters and cosmological implications. Monthly Notices of the Royal Astronomical Society, 385 (4). pp. 2243-2253. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:ANDmnras08

[img]
Preview
PDF - Published Version
See Usage Policy.

222Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:ANDmnras08

Abstract

Cosmic rays produced in cluster accretion and merger shocks provide pressure to the intracluster medium (ICM) and affect the mass estimates of galaxy clusters. Although direct evidence for cosmic ray ions in the ICM is still lacking, they produce γ -ray emission through the decay of neutral pions produced in their collisions with ICM nucleons. We investigate the capability of the Gamma-ray Large Area Space Telescope (GLAST) and imaging atmospheric Cêrenkov telescopes (IACTs) for constraining the cosmic ray pressure contribution to the ICM. We show that GLAST can be used to place stringent upper limits, a few per cent for individual nearby rich clusters, on the ratio of pressures of the cosmic rays and thermal gas. We further show that it is possible to place tight (≤ 10 per cent) constraints for distant (z ≤ 0.25) clusters in the case of hard spectrum, by stacking signals from samples of known clusters. The GLAST limits could be made more precise with the constraint on the cosmic ray spectrum potentially provided by IACTs. Future γ-ray observations of clusters can constrain the evolution of cosmic ray energy density, which would have important implications for cosmological tests with upcoming X-ray and Sunyaev–Zel’dovich effect cluster surveys.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1111/j.1365-2966.2008.12996.xDOIArticle
ORCID:
AuthorORCID
Nagai, Daisuke0000-0002-6766-5942
Additional Information:© 2008 The Authors. Journal compilation RAS, MNRAS. Accepted 2008 January 19. Received 2007 December 19; in original form 2007 May 16. We thank Christoph Pfrommer, Julie McEnery and Steven Ritz for useful comments. This work was supported by Sherman Fairchild Foundation.
Funders:
Funding AgencyGrant Number
Sherman Fairchild FoundationUNSPECIFIED
Subject Keywords:radiation mechanisms: non-thermal; cosmic rays; galaxies: clusters: general; cosmology: miscellaneous; gamma-rays: theory.
Issue or Number:4
Record Number:CaltechAUTHORS:ANDmnras08
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:ANDmnras08
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:13434
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:18 Aug 2009 17:35
Last Modified:20 Nov 2019 22:25

Repository Staff Only: item control page