Study of warm inflation using irreversible thermodynamical description within Rastall gravity

2021 ◽  
pp. 100920
Author(s):  
R. Saleem ◽  
Iqra Shahid
Keyword(s):  
2017 ◽  
Vol 77 (11) ◽  
Author(s):  
Abdul Jawad ◽  
Shahid Chaudhary ◽  
Nelson Videla
Keyword(s):  

2021 ◽  
pp. 100938
Author(s):  
Akash Bose ◽  
Subenoy Chakraborty
Keyword(s):  

2007 ◽  
Vol 653 (2-4) ◽  
pp. 122-128 ◽  
Author(s):  
Sergio del Campo ◽  
Ramón Herrera

Universe ◽  
2020 ◽  
Vol 6 (6) ◽  
pp. 74
Author(s):  
Zbigniew Haba

The time-dependent cosmological term arises from the energy-momentum tensor calculated in a state different from the ground state. We discuss the expectation value of the energy-momentum tensor on the right hand side of Einstein equations in various (approximate) quantum pure as well as mixed states. We apply the classical slow-roll field evolution as well as the Starobinsky and warm inflation stochastic equations in order to calculate the expectation value. We show that, in the state concentrated at the local maximum of the double-well potential, the expectation value is decreasing exponentially. We confirm the descent of the expectation value in the stochastic inflation model. We calculate the cosmological constant Λ at large time as the expectation value of the energy density with respect to the stationary probability distribution. We show that Λ ≃ γ 4 3 where γ is the thermal dissipation rate.


2017 ◽  
Vol 14 (06) ◽  
pp. 1750093 ◽  
Author(s):  
Lorenzo Sebastiani ◽  
Ratbay Myrzakulov

In this paper, [Formula: see text]-inflation is analyzed in warm braneworld scenario. A general class of [Formula: see text]-essence models with power-law kinetic term is investigated and weak and strong dissipation regimes are studied. Scalar perturbations and spectral index are derived. The results are discussed and applied to specific examples.


2016 ◽  
Vol 2016 (03) ◽  
pp. 059-059 ◽  
Author(s):  
Xiao-Min Zhang ◽  
Hong-Yang Ma ◽  
Peng-Cheng Chu ◽  
Jun-Ting Liu ◽  
Jian-Yang Zhu
Keyword(s):  

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