The large-scale structure formation in an expanding universe

Author:

Hameeda Mir12,Pourhassan Behnam3,Masood Syed4,Faizal Mir567,Wang Li-Gang4,Abass Shohaib8

Affiliation:

1. Department of Physics, S.P. Collage, Srinagar 190001, Kashmir, India

2. Inter University Centre for Astronomy and Astrophysics, Pune, India

3. School of Physics, Damghan University, Damghan 3671641167, Iran

4. Zhejiang Province Key Laboratory of Quantum Technology and Device, Department of Physics, Zhejiang University, Hangzhou 310027, P. R. China

5. Irving K. Barber School of Arts and Sciences, University of British Columbia, Kelowna, British Columbia, Canada V1V 1V7, Canada

6. Department of Physics and Astronomy, University of Lethbridge, Lethbridge, Alberta, Canada T1K 3M4, Canada

7. Canadian Quantum Research Center, 204-3002 32 Ave Vernon, Canada BC V1T 2L7, Canada

8. Department of Physics, Central University of Kashmir, Tulmulla Campus Ganderbal 191131, Kashmir, India

Abstract

In this paper, we analyze the effects of expansion on large-scale structure formation in our universe. We do that by incorporating a cosmological constant term in the gravitational partition function. This gravitational partition function with a cosmological constant is used for analyzing the thermodynamics of this system. We analyze the virial expansion for this system, and obtain its equation of state. It is observed that the generalization of this equation of state is like the Van der Waals equation. We also analyze a gravitational phase transition in this system using the mean-field theory. We construct the cosmic energy equation for this system of galaxies, and discuss its consequences. We obtain and analyze the distribution function for this system, using the gravitational partition function. We also compare the results obtained in this paper with the observational data.

Publisher

World Scientific Pub Co Pte Ltd

Subject

Astronomy and Astrophysics,Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics

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