activity
20032026
most citedCosmological Constraints on a Power Law Universe

68 citations · 120 across the 9 of their papers we have counts for

collaborators

9 papers

physics.gen-ph2026

Growth-of-Structure Constraints on the Variable Chaplygin Gas Model

Rishabh Jain, Shruti Thakur, Geetanjali Sethi

A unified description of dark matter and the late-time acceleration of the Universe offers an attractive framework for explaining the dark sector. Among such models, the Variable C…

astro-ph.EP2024★ 2 cited

Studying habitability of the exoplanets Kepler-504 b, Kepler-315 b, and Kepler-315 c

Sattik Bhaumik, Geetanjali Sethi

Astronomers have always wanted to know whether there are other planets around other stars that support life like our Earth. The search for life elsewhere has led us to new findings…

astro-ph.CO2023

Variable Chaplygin Gas: Contraining parameters using FRBs

Geetanjali Sethi, Udish Sharma, Nadia Makhijani

We investigate cosmological constraints on the Variable Chaplygin gas model parameters with latest observational data of the Fast Radio Bursts and compare the results with previous…

astro-ph.CO2022★ 6 cited

Variable Chaplygin Gas: Constraints from Supernovae, GRB and Gravitational Wave Merger Events

Ashley Chraya, Yuvraj Muralichandran, Geetanjali Sethi

We investigate the cosmological constraints on the Variable Chaplygin gas model from the latest observational data: SCP Union 2.1 compilation dataset of Type Ia supernovae (SNe Ia)…

astro-ph.CO2014★ 1 cited

Variable Chaplygin Gas: Constraints from Supernovae, BAO, Look Back Time, and GRBs

Bhuvan Aggarwal, Geetanjali Sethi, Shruti Thakur

We examine the variable Chaplygin gas (VCG) model with the aim of establishing tight constraints by using type-Ia supernovae, lookback time measurements, Baryon Acoustic Oscillatio…

astro-ph2005★ 27 cited

Variable Chaplygin Gas: Constraints from CMBR and SNe Ia

Geetanjali Sethi, Sushil K. Singh, Pranav Kumar +2

We constrain the parameters of the variable Chaplygin gas model, using the location of peaks of the CMBR spectrum and SNe Ia ``gold '' data set. Equation of state of the model is $…