scholarly journals FIMP Dark Matter from Leptogenesis in Fast Expanding Universe

2021 ◽  
Vol 2021 (06) ◽  
pp. 006
Author(s):  
Zhi-Fang Chang ◽  
Zhao-Xuan Chen ◽  
Jia-Shu Xu ◽  
Zhi-Long Han
1995 ◽  
Vol 48 (6) ◽  
pp. 1083 ◽  
Author(s):  
PJ Quinn

N-body models running on supercomputers have been widely used to explore the development of structure in the expanding Universe. Recent results from the COBE satellite have provided a global normalisation of these models which now allows detailed comparisons to be drawn between observations and model predictions. Some predictions of the cold dark matter primordial perturbation spectrum are now shown to be consistent with surveys of galaxy redshifts.


2015 ◽  
Vol 5 (1) ◽  
pp. 51-56 ◽  
Author(s):  
M. Tsizh ◽  
B. Novosyadlyj

We investigate the non-linear evolution of spherical density and velocity perturbations of dark matter and dark energy in the expanding Universe. For this we have used the conservation and Einstein equations to describe the evolution of gravitationally coupled inhomogeneities of dark matter, dark energy and radiation from the linear stage in the early Universe to the non-linear stage at the current epoch. A simple method of numerical integration of the system of non-linear differential equations for evolution of the central part of halo is proposed. The results are presented for the halo of cluster (k=2 Mpc-1) and supercluster scales (k=0.2 Mpc-1) and show that a quintessential scalar field dark energy with a low value of effective speed of sound cs<0.1 can have a notable impact on the formation of large-scale structures in the expanding Universe.


2014 ◽  
Vol 355 (1) ◽  
pp. 187-193 ◽  
Author(s):  
En-Kun Li ◽  
Yu Zhang ◽  
Jin-Ling Geng ◽  
Peng-Fei Duan

2010 ◽  
Vol 2010 ◽  
pp. 1-14 ◽  
Author(s):  
Tong-Jie Zhang ◽  
Cong Ma ◽  
Tian Lan

This paper is a review on the observational Hubble parameter data that have gained increasing attention in recent years for their illuminating power on the dark side of the universe: the dark matter, dark energy, and the dark age. Currently, there are two major methods of independent observationalH(z)measurement, which we summarize as the “differential age method” and the “radial BAO size method.” Starting with fundamental cosmological notions such as the spacetime coordinates in an expanding universe, we present the basic principles behind the two methods. We further review the two methods in greater detail, including the source of errors. We show how the observationalH(z)data present itself as a useful tool in the study of cosmological models and parameter constraint, and we also discuss several issues associated with their applications. Finally, we point the reader to a future prospect of upcoming observation programs that will lead to some major improvements in the quality of observationalH(z)data.


2021 ◽  
Vol 104 (1) ◽  
Author(s):  
Basabendu Barman ◽  
Purusottam Ghosh ◽  
Farinaldo S. Queiroz ◽  
Abhijit Kumar Saha

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