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15 papers · 1 filter
Subluminal OPERA Neutrinos
Ichiro Oda
The OPERA collaboration has announced to have observed superluminal neutrinos with a mean energy 17.5 GeV, but afterward the superluminal interpretation of the OPERA results has be…
Superluminal Neutrinos from Gauge Field
Ichiro Oda, Hajime Taira
We consider a possibility that the recent OPERA results on neutrinos' superluminality could be caused by a local effect of a new gauge field sourced by the earth. If neutrinos coup…
Quasi-equilibrium models of magnetized compact objects
Charalampos Markakis, Koji Uryu, Eric Gourgoulhon
We report work towards a relativistic formulation for modeling strongly magnetized neutron stars, rotating or in a close circular orbit around another neutron star or black hole, u…
A Resolution to Cherenkov-like Radiation of OPERA Neutrinos
Ichiro Oda, Hajime Taira
The OPERA collabotation has reported evidence of superluminal neutrinos with a mean energy 17.5 GeV ranging up to 50 GeV. However, the superluminal interpretation of the OPERA resu…
Neutron star equation of state via gravitational wave observations
Charalampos Markakis, Jocelyn S. Read, Masaru Shibata +4
Gravitational wave observations can potentially measure properties of neutron star equations of state by measuring departures from the point-particle limit of the gravitational wav…
Implementing Continuation based language in GCC
Shinji Kono, Kento Yogi
We have implemented C like Continuation based programming language. Continuation based C, CbC was implemented using micro-C on various architecture, and we have tried several CbC p…