Cosmic evolution in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si381.svg" display="inline" id="d1e2636"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>Q</mml:mi><mml:mo>,</mml:mo><mml:mi>T</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> gravity: Exploring a higher-order time-dependent function of deceleration parameter with observational constraints-Reference-Cited by-同舟云学术

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Cosmic evolution in f(Q,T) gravity: Exploring a higher-order time-dependent function of deceleration parameter with observational constraints

Published:2024-02 Issue: Volume:43 Page:101408
ISSN:2212-6864
Container-title:Physics of the Dark Universe
language:en
Short-container-title:Physics of the Dark Universe

Author:

Khurana Madhur^ORCID,Chaudhary Himanshu,Mumtaz Saadia,Pacif S.K.J.,Mustafa G.

Funder

Zhejiang Normal University

Department of Physics, Harvard University

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference157 articles.

1. Measurements of Ω and Λ from 42 high-redshift supernovae;Perlmutter;Astrophys. J.,1999

2. Observational evidence from supernovae for an accelerating universe and a cosmological constant;Riess;Astron. J.,1998

3. Dark interactions and cosmological fine-tuning;Quartin;J. Cosmol. Astropart. Phys.,2008

4. Unitary evolution and cosmological fine-tuning;Carroll,2010

5. Aspects of the cosmological “coincidence problem”;Velten;Eur. Phys. J. C,2014

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