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most citedEstimation of Cosmological Parameters from HI Observations of Post-reionization Epoch

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astro-ph200850 cited

Estimation of Cosmological Parameters from HI Observations of Post-reionization Epoch

Somnath Bharadwaj, Shiv K. Sethi, Tarun Deep Saini

The emission from neutral hydrogen (HI) clouds in the post-reionization era (z < 6), too faint to be individually detected, is present as a diffuse background in all low frequency…

astro-ph2005

Cosmology with decaying tachyon matter

A. Das, Shashikant Gupta, Tarun Deep Saini +1

We investigate the case of a homogeneous tachyon field coupled to gravity in a spatially flat Friedman-Robertson-Walker spacetime. Assuming the field evolution to be exponentially…

astro-ph2003

Is there Supernova Evidence for Dark Energy Metamorphosis ?

Ujjaini Alam, Varun Sahni, Tarun Deep Saini +1

We reconstruct the equation of state of dark energy (DE) using a recently released data set containing 172 type Ia supernovae without assuming the prior (in c…

astro-ph2003

Revealing the Nature of Dark Energy Using Bayesian Evidence

T. D. Saini, J. Weller, S. L. Bridle

We apply the Bayesian concept of `evidence' to reveal systematically the nature of dark energy from present and future supernova luminosity distance measurements. We express the un…

astro-ph2003

Exploring the Expanding Universe and Dark Energy using the Statefinder Diagnostic

Ujjaini Alam, Varun Sahni, Tarun Deep Saini +1

The coming few years are likely to witness a dramatic increase in high quality Sn data as current surveys add more high redshift supernovae to their inventory and as newer and deep…

astro-ph2003

Response of distance measures to the equation of state

Tarun Deep Saini, T. Padmanabhan, Sarah Bridle

We show that the distance measures (such as the luminosity and angular diameter distances) are linear functionals of the equation-of-state function w(z) of the dark energy to a fai…