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most citedNeutrino-Nucleus Reaction Cross Sections for Light Element Synthesis in Supernova Explosions

107 citations · 461 across the 8 of their papers we have counts for

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astro-ph2008107 cited

Neutrino-Nucleus Reaction Cross Sections for Light Element Synthesis in Supernova Explosions

T. Yoshida, T. Suzuki, S. Chiba +5

The neutrino-nucleus reaction cross sections of 4He and 12C are evaluated using new shell model Hamiltonians. Branching ratios of various decay channels are calculated to evaluate…

astro-ph200834 cited

New Constraints on Radiative Decay of Long-Lived Particles in Big Bang Nucleosynthesis with New He Photodisintegration Data

Motohiko Kusakabe, Toshitaka Kajino, Takashi Yoshida +3

A recent measurement of He photodisintegration reactions, He(,)H and He(,)He with laser-Compton photons shows smaller cross sections than those esti…

astro-ph200762 cited

A Simultaneous Solution to the ^6Li and ^7Li Big Bang Nucleosynthesis Problems from a Long-Lived Negatively-Charged Leptonic Particle

Motohiko Kusakabe, Toshitaka Kajino, Richard N. Boyd +2

The Li abundance observed in metal poor halo stars exhibits a plateau similar to that for Li suggesting a primordial origin. However, the observed abundance of Li is a…

astro-ph200646 cited

Neutrino Oscillation Effects on Supernova Light Element Synthesis

T. Yoshida, T. Kajino, H. Yokomakura +3

Neutrino oscillations affect light element synthesis through the neutrino-process in supernova explosions. The 7Li and 11B yields produced in a supernova explosion of a 16.2 solar-…

astro-ph200678 cited

Supernova Neutrino Nucleosynthesis of Light Elements with Neutrino Oscillations

T. Yoshida, T. Kajino, H. Yokomakura +3

Light element synthesis in supernovae through neutrino-nucleus interactions, i.e., the nu-process, is affected by neutrino oscillations in the supernova environment. There is a res…

astro-ph2005

Constraining the Spectrum of Supernova Neutrinos from Neutrino-Process-Induced Light-Element Synthesis

Takashi Yoshida, Toshitaka Kajino, Dieter H. Hartmann

We constrain energy spectra of supernova neutrinos through the avoidance of an overproduction of the 11B abundance during Galactic chemical evolution. In supernova nucleosynthesis…