activity
20102022
most citedObservational constraints on phantom power-law cosmology

27 citations · 71 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2022★ 16 cited

Observational constraints on interacting vacuum energy with linear interactions

Chakkrit Kaeonikhom, Hooshyar Assadullahi, Jascha Schewtschenko +1

We explore the bounds that can be placed on interactions between cold dark matter and vacuum energy, with equation of state , using state-of-the-art cosmological observations…

astro-ph.CO2020★ 8 cited

Qualitative dynamics of interacting vacuum cosmologies

Chakkrit Kaeonikhom, Phongsaphat Rangdee, Hooshyar Assadullahi +3

We present a phase-space analysis of the qualitative dynamics cosmologies where dark matter exchanges energy with the vacuum component. We find fixed points corresponding to power-…

astro-ph.CO2018

Redshift-space distortion from dynamical dark energy with time-dependent Lagrangian perturbation theory

Chakkrit Kaeonikhom, Teeraparb Chantavat

We apply the Lagrangian perturbation theory with time-dependent growth functions at second and third order of perturbation with the aim to model the effect of dynamical dark energy…

gr-qc2012★ 19 cited

Dynamics of Dirac-Born-Infeld dark energy interacting with dark matter

Chakkrit Kaeonikhom, Douglas Singleton, Sergey V. Sushkov +1

We study the dynamics of Dirac-Born-Infeld (DBI) dark energy interacting with dark matter. The DBI dark energy model considered here has a scalar field with a nonstandard kinetic e…

astro-ph.CO2012★ 1 cited

WMAP7 constraints on scalar-field power-law cosmology

Burin Gumjudpai, Chakkrit Kaeonikhom

In this paper, power-law cosmology whose scale factor is a power of time, $a \propto t^{\a}$, is investigated. Considering late universe with canonical scalar field and dust domina…

astro-ph.CO2010★ 27 cited

Observational constraints on phantom power-law cosmology

Chakkrit Kaeonikhom, Burin Gumjudpai, Emmanuel N. Saridakis

We investigate phantom cosmology in which the scale factor is a power law, and we use cosmological observations from Cosmic Microwave Background (CMB), Baryon Acoustic Oscillations…