Ушбу ишга иқтибос қилган ишлар

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Иш: Seven Hints That Early-Time New Physics Alone Is Not Sufficient to Solve the Hubble Tension

1. 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

   Madhur Khurana, Himanshu Chaudhary, Saadia Mumtaz +2

   МақолаCosmology and Gravitation TheoriesPhysics of the Dark Universe20233 иқтибос

   ABIABI:AkademIndex/openalex/2023.article.000166

2. Extracting H0 and r in q(t) parametrization models

   Himanshu Chaudhary, S. K. J. Pacif, G. Mustafa +2

   МақолаTensor decomposition and applicationsJournal of High Energy Astrophysics20253 иқтибос

   ABIABI:AkademIndex/openalex/2025.article.000339

3. Addressing the r tension using late-time observational measurements in a novel deceleration parametrization

   Himanshu Chaudhary, Ujjal Debnath, S. K. Maurya +2

   МақолаCosmology and Gravitation TheoriesJournal of High Energy Astrophysics20240 иқтибос

   ABIABI:AkademIndex/openalex/2024.article.002600

4. Dark sector interactions: Probing the Hubble parameter and the sound horizon

   Ritika Nagpal, S. K. J. Pacif, Farruh Atamurotov +1

   МақолаCosmology and Gravitation TheoriesAnnals of Physics20250 иқтибос

   ABIABI:AkademIndex/openalex/2025.article.001391