Study of the large scale structure through modified gravity theory using statistical mechanics

被引：1
作者：
Khanday, Abdul W. [1 ]
Upadhyay, Sudhaker [2 ,3 ,4 ,5 ]
Ganai, Prince A. [1 ]
机构：
[1] Natl Inst Technol Srinagar, Dept Phys, Srinagar 190006, Jammu & Kashmir, India
[2] KLS Coll, Dept Phys, Nawada 805110, Bihar, India
[3] Magadh Univ, Dept Phys, Bodh Gaya 824234, Bihar, India
[4] Interuniv Ctr Astron & Astrophys IUCAA Pune, Pune 411007, Maharashtra, India
[5] Damghan Univ, Sch Phys, Damghan 3671641167, Iran
来源：
PHYSICA A-STATISTICAL MECHANICS AND ITS APPLICATIONS | 2023年 / 612卷
关键词：
Galaxy clusters; Statistical mechanics; Thermodynamics; Distribution functions; Data analysis; SDSS; GALAXIES;
D O I：
10.1016/j.physa.2023.128493
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
We discuss the galaxy clustering based on thermodynamics and statistical mechanics in the expanding universe in a modified theory of gravity. The modified general relativity (MGR) is developed using the regular line element field to construct a symmetric tensor that represents the energy momentum of the gravitational field. This in turn provides a modified gravitational potential with terms that represent dark matter and dark energy effects without actually invoking the two. Based on the modified gravitational potential we calculate the distribution function of the galaxies. We also calculate various thermodynamic equations of state. We make a data analysis of the data obtained through the SDSS-III survey and check the feasibility of the theoretical model of probability distribution of galaxies in the universe. (c) 2023 Elsevier B.V. All rights reserved.
引用
收藏
页数：13
相关论文
共 23 条
[1]   Statistical mechanics of the cosmological many-body problem [J].
Ahmad, F ;
Saslaw, WC ;
Bhat, NI .
ASTROPHYSICAL JOURNAL, 2002, 571 (02) :576-584
[2]  
Qadri DA, 2022, Arxiv, DOI arXiv:2206.15173
[3]   The formation of the first stars and galaxies [J].
Bromm, Volker ;
Yoshida, Naoki ;
Hernquist, Lars ;
McKee, Christopher F. .
NATURE, 2009, 459 (7243) :49-54
[4]   Clustering of galaxies with f(R) gravity [J].
Capozziello, Salvatore ;
Faizal, Mir ;
Hameeda, Mir ;
Pourhassan, Behnam ;
Salzano, Vincenzo ;
Upadhyay, Sudhaker .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2018, 474 (02) :2430-2443
[5]   Extended Theories of Gravity [J].
Capozziello, Salvatore ;
De Laurentis, Mariafelicia .
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 2011, 509 (4-5) :167-320
[6]   Modified theory of gravity and clustering of multi-component system of galaxies [J].
Hameeda, Mir ;
Pourhassan, Behnam ;
Faizal, Mir ;
Masroor, C. P. ;
Ansari, Rizwan Ul Haq ;
Suresh, P. K. .
EUROPEAN PHYSICAL JOURNAL C, 2019, 79 (09)
[7]   Large distance modification of Newtonian potential and structure formation in universe [J].
Hameeda, Mir ;
Upadhyay, Sudhaker ;
Faizal, Mir ;
Ali, Ahmed F. ;
Pourhassan, Behnam .
PHYSICS OF THE DARK UNIVERSE, 2018, 19 :137-143
[8]   Effects of cosmological constant on clustering of Galaxies [J].
Hameeda, Mir ;
Upadhyay, Sudhaker ;
Faizal, Mir ;
Ali, Ahmed Farag .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2016, 463 (04) :3699-3704
[9]   EVOLUTION AND CLUSTERING OF RICH CLUSTERS [J].
KAISER, N .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1986, 222 (02) :323-345
[10]  
Khanday AW, 2023, Arxiv, DOI arXiv:2203.17237
123