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20112026
most citedComposite Models for the 750 GeV Diphoton Excess

199 citations · 4.2k across the 135 of their papers we have counts for

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6 papers · 1 filter

astro-ph.CO2020★ 42 cited

Increasing Temperature toward the Completion of Reheating

Raymond T. Co, Eric Gonzalez, Keisuke Harigaya

Reheating is a process where the energy density of a dominant component of the universe other than radiation, such as a matter component, is transferred into radiation. It is usual…

astro-ph.CO2019★ 3 cited

Common Origin of Warm Dark Matter and Dark Radiation

Manuel A. Buen-Abad, Raymond T. Co, Keisuke Harigaya

We consider a cosmological scenario where a relativistic particle and a stable massive particle are simultaneously produced from the decay of a late-decaying particle after Big-Ban…

astro-ph.CO2018★ 3 cited

New Inflation in the Landscape and Typicality of the Observed Cosmic Perturbation

Chien-I Chiang, Keisuke Harigaya

We investigate if the observed small and nearly scale-invariant primordial cosmic perturbation, i.e. the perturbation amplitude and the spectral index $n_s \simeq…

astro-ph.CO2016★ 8 cited

Hubble induced mass after inflation in spectator field models

Tomohiro Fujita, Keisuke Harigaya

Spectator field models such as the curvaton scenario and the modulated reheating are attractive scenarios for the generation of the cosmic curvature perturbation, as the constraint…

astro-ph.CO2014★ 192 cited

Baryon Asymmetry, Dark Matter, and Density Perturbation from PBH

Tomohiro Fujita, Keisuke Harigaya, Masahiro Kawasaki +1

We investigate the consistency of a scenario in which the baryon asymmetry, dark matters, as well as the cosmic density perturbation are generated simultaneously through the evapor…

astro-ph.CO2013★ 6 cited

Large Scale Cosmic Perturbation from Evaporation of Primordial Black Holes

Tomohiro Fujita, Keisuke Harigaya, Masahiro Kawasaki

We present a novel mechanism to generate the cosmic perturbation from evaporation of primordial black holes. A mass of a field is fluctuated if it is given by a vacuum expectation…