output
19932026
most citedPrimordial Black Hole Scenario for the Gravitational-Wave Event GW150914

934 citations

Showing 2019 · gr-qcShow all

21 papers · 2 filters

gr-qc2019★ 15 cited

Relativistic stars in a cubic Galileon Universe

Hiromu Ogawa, Tsutomu Kobayashi, Kazuya Koyama

We study relativistic stars in Hordenski theories that evade the gravitational wave constraints and exhibit the Vainshtein mechanism, focusing on a model based on the cubic Galileo…

gr-qc2019★ 17 cited

Revisiting slow-roll dynamics and the tensor tilt in general single-field inflation

Yosuke Mishima, Tsutomu Kobayashi

We explore the possibility of a blue-tilted gravitational wave spectrum from potential-driven slow-roll inflation in the Horndeski theory. In Kamada et al. (2012), it was claimed t…

gr-qc2019★ 74 cited

On the gauge dependence of gravitational waves generated at second order from scalar perturbations

Keitaro Tomikawa, Tsutomu Kobayashi

We revisit and clarify the gauge dependence of gravitational waves generated at second order from scalar perturbations. In a universe dominated by a perfect fluid with a constant e…

gr-qc2019★ 20 cited

Escape probability of a photon emitted near the black hole horizon

Kota Ogasawara, Takahisa Igata, Tomohiro Harada +1

We investigate the escape of photons from the vicinity of the horizon to infinity in the Kerr-Newmann black hole spacetime. We assume that a light source is at rest in a locally no…

gr-qc2019★ 24 cited

Primordial non-Gaussianities of scalar and tensor perturbations in general bounce cosmology: Evading the no-go theorem

Shingo Akama, Shin'ichi Hirano, Tsutomu Kobayashi

It has been pointed out that matter bounce cosmology driven by a k-essence field cannot satisfy simultaneously the observational bounds on the tensor-to-scalar ratio and non-Gaussi…

gr-qc2019★ 2 cited

Dynamical Transition from a Naked Singularity to a Black Hole

Kenta Hioki, Tomohiro Harada

We show that a Reissner-Nordström (RN) black hole can be formed by dropping a charged thin dust shell onto a RN naked singularity. This is in contrast to the fact that a RN naked s…