activity
20182021
most citedTrans-Planckian censorship and single-field inflaton potential

29 citations · 44 across the 3 of their papers we have counts for

collaborators

10 papers

gr-qc202111 cited

Primordial black holes and induced gravitational waves from inflation in the Horndeski theory of gravity

Pisin Chen, Seoktae Koh, Gansukh Tumurtushaa

We investigate the production of primordial black holes (PBHs) and scalar-induced gravitational waves (GWs) for cosmological models in the Horndeski theory of gravity. The cosmolog…

astro-ph.CO2021

Observational Constraints on the Cosmology with Holographic Dark Fluid

Da Huang, Bum-Hoon Lee, Gansukh Tumurtushaa +2

We consider the holographic Friedman-Robertson-Walker (hFRW) universe on the 4-dimensional membrane embedded in the 5-dimensional bulk spacetime and fit the parameters with the obs…

gr-qc20204 cited

Euclidean wormholes in Gauss-Bonnet-dilaton gravity

Xiao Yan Chew, Gansukh Tumurtushaa, Dong-han Yeom

We investigate Euclidean wormholes in Gauss-Bonnet-dilaton gravity to explain the creation of the universe from nothing. We considered two types of dilaton couplings (i.e., the str…

gr-qc2020

Constraints on dark energy models from the Horndeski theory

Bilguun Bayarsaikhan, Seoktae Koh, Enkhbat Tsedenbaljir +1

In light of the cosmological observations, we investigate dark energy models from the Horndeski theory of gravity. In particular, we consider cosmological models with the derivativ…

astro-ph.CO2020

The viable f(G) gravity models via reconstruction from the observations

Seokcheon Lee, Gansukh Tumurtushaa

We reconstruct the viable f(G) gravity models from the observations and provide the analytic solutions that well describe our numerical results. In order to avoid unphysical challe…

hep-th201929 cited

Trans-Planckian censorship and single-field inflaton potential

Kenji Kadota, Chang Sub Shin, Takahiro Terada +1

It was recently proposed that a field theory cannot be consistent with quantum gravity if it allows a mode shorter than the Planck length to exit the Hubble horizon. This is called…