output
19922026
most citedObservation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC

10.9k citations

Showing 2016 · astro-ph.HEShow all

11 papers · 2 filters

astro-ph.HE2016★ 13 cited

On a role of corotation radius in the low dynamical instability of differentially rotating stars

Shin'ichirou Yoshida, Motoyuki Saijo

We investigate the nature of so-called low dynamical instability in a differentially rotating star by focusing on the role played by the corotation radius of the unstable osc…

astro-ph.HE2016★ 189 cited

The intermediate r-process in core-collapse supernovae driven by the magneto-rotational instability

Nobuya Nishimura, Hidetomo Sawai, Tomoya Takiwaki +2

We investigated r-process nucleosynthesis in magneto-rotational supernovae, based on a new explosion mechanism induced by the magneto-rotational instability. A series of axisymmetr…

astro-ph.HE2016★ 22 cited

High-Energy Non-Thermal and Thermal Emission from GRB141207A detected by Fermi

Makoto Arimoto, Katsuaki Asano, Masanori Ohno +5

The bright long gamma-ray burst GRB 141207A was observed by the {\it Fermi Gamma-ray Space Telescope} and detected by both instruments onboard. The observations show that the spect…

astro-ph.HE2016★ 5 cited

Rotational equilibria by Lagrangian variational principle: toward multi-dimensional stellar evolutions

Nobutoshi Yasutake, Kotaro Fujisawa, Shoichi Yamada

We have developed a new formulation to obtain self-gravitating, axisymmetric configurations in permanent rotation. The formulation is based on the Lagrangian variational principle…

astro-ph.HE2016★ 124 cited

Hitomi constraints on the 3.5 keV line in the Perseus galaxy cluster

Hitomi Collaboration, Felix A. Aharonian, Hiroki Akamatsu +215

High-resolution X-ray spectroscopy with Hitomi was expected to resolve the origin of the faint unidentified E=3.5 keV emission line reported in several low-resolution studies of va…

astro-ph.HE2016★ 23 cited

CALET Upper Limits on X-ray and Gamma-ray Counterparts of GW 151226

O. Adriani, Y. Akaike, K. Asano +89

We present upper limits in the hard X-ray and gamma-ray bands at the time of the LIGO gravitational-wave event GW 151226 derived from the CALorimetric Electron Telescope (CALET) ob…

astro-ph.HE2016★ 26 cited

Inverse Compton X-ray Emissions from TeV blazar Mrk421 during a Historical Low-Flux State Observed with NuSTAR

Jun Kataoka, Lukasz Stawarz

We report on the detection of excess hard X-ray emission from the TeV BL Lac object Mrk421 during the historical low-flux state of the source in January 2013. NuSTAR observations w…

astro-ph.HE2016★ 33 cited

Circular polarizations of gravitational waves from core-collapse supernovae: a clear indication of rapid rotation

Kazuhiro Hayama, Takami Kuroda, Ko Nakamura +1

We propose to employ the circular polarization of gravitational waves emitted by core-collapse supernovae as an unequivocal indication of rapid rotation deep in their cores. It has…

astro-ph.HE2016★ 67 cited

Three-dimensional Boltzmann-Hydro code for core-collapse in massive stars II. The Implementation of moving-mesh for neutron star kicks

Hiroki Nagakura, Wakana Iwakami, Shun Furusawa +4

We present a newly developed moving-mesh technique for the multi-dimensional Boltzmann-Hydro code for the simulation of core-collapse supernovae (CCSNe). What makes this technique…

astro-ph.HE2016★ 23 cited

Links between the shock instability in core-collapse supernovae and asymmetric accretions of envelopes

Kazuya Takahashi, Wakana Iwakami, Yu Yamamoto +1

The explosion mechanism of core-collapse supernovae has not been fully understood yet but multi-dimensional fluid instabilities such as standing accretion shock instability (SASI)…

astro-ph.HE2016★ 132 cited

Multi-messenger signals of long-term core-collapse supernova simulations : synergetic observation strategies

Ko Nakamura, Shunsaku Horiuchi, Masaomi Tanaka +3

The next Galactic supernova is expected to bring great opportunities for the direct detection of gravitational waves (GW), full flavor neutrinos, and multi-wavelength photons. To m…