Searching for deviations from the General Relativity Theory with gas mass fraction of galaxy clusters and complementary probes

التفاصيل البيبلوغرافية
العنوان: Searching for deviations from the General Relativity Theory with gas mass fraction of galaxy clusters and complementary probes
المؤلفون: Holanda, R. F. L., Pereira, S. H., Santos-da-Costa, S.
المصدر: Phys. Rev. D 95, 084006 (2017)
سنة النشر: 2016
المجموعة: Astrophysics
General Relativity and Quantum Cosmology
مصطلحات موضوعية: Astrophysics - Cosmology and Nongalactic Astrophysics, General Relativity and Quantum Cosmology
الوصف: Nowadays, thanks to the improved precision of cosmological data, it has been possible to search for deviation from the general relativity theory with tests on large cosmic scales. Particularly, there is a class of modified gravity theories that breaks the Einstein equivalence principle (EEP) in the electromagnetic sector, generating variations of the fine structure constant, violations of the cosmic distance duality relation and the evolution law of the cosmic microwave background (CMB) radiation. In recent papers, this class of theories has been tested with angular diameter distances from galaxy clusters, type Ia supernovae and CMB temperature. In this work we propose a new test by considering the most recent X-ray surface brightness observations of galaxy clusters jointly with type Ia supernovae and CMB temperature. {The crucial point here is that we take into account the dependence of the X-ray gas mass fraction of galaxy clusters on possible variations of the fine structure constant and violations of the cosmic distance duality relation.} Our basic result is that this new approach is competitive with the previous one and it also does not show significant deviations from the general relativity.
Comment: 8 pages, 2 figures. Accepted for publication in Physical Review D. The authors thank the anonymous referee for the valuable suggestions
نوع الوثيقة: Working Paper
DOI: 10.1103/PhysRevD.95.084006
URL الوصول: http://arxiv.org/abs/1612.09365
رقم الأكسشن: edsarx.1612.09365
قاعدة البيانات: arXiv
الوصف
DOI:10.1103/PhysRevD.95.084006