activity
19932026
most citedNucleosynthetic signatures of the first stars

566 citations · 7.6k across the 203 of their papers we have counts for

collaborators
Showing 2012Show all

6 papers · 1 filter

astro-ph.IM2012★ 13 cited

The JEM-EUSO Mission: Status and Prospects in 2011

EUSO Collaboration, J. H. Adams, S. Ahmad +256

Contributions of the JEM-EUSO Collaboration to the 32nd International Cosmic Ray Conference, Beijing, August, 2011.

nucl-th2012★ 83 cited

Neutrino Capture on C

T. Suzuki, A. B. Balantekin, T. Kajino

We present neutrino cross sections on C. The charged-current cross sections leading to various states in the daughter and the neutral-current cross sections leading…

astro-ph.CO2012★ 74 cited

The Search for a Primordial Magnetic Field

Dai G. Yamazaki, Toshitaka Kajino, Grant J. Mathew +1

Magnetic fields appear wherever plasma and currents can be found. As such, they thread through all scales in Nature. It is natural, therefore, to suppose that magnetic fields might…

astro-ph.SR2012★ 41 cited

Impact of New beta-decay Half-lives on r-process Nucleosynthesis

Nobuya Nishimura, Toshitaka Kajino, Grant J. Mathews +2

We investigate the effects of newly measured beta-decay half-lives on r-process nucleosynthesis. These new rates were determined by recent experiments at the radioactive isotope be…

astro-ph.CO2012★ 20 cited

Solution to Big-Bang Nucleosynthesis in Hybrid Axion Dark Matter Model

Motohiko Kusakabe, A. B. Balantekin, Toshitaka Kajino +1

Following a recent suggestion of axion cooling of photons between the nucleosynthesis and recombination epochs in the Early Universe, we investigate a hybrid model with both axions…

astro-ph.HE2012★ 19 cited

Relativistic Mean-Field Treatment of Pulsar Kick from Neutrino Propagation in Magnetized Proto-Neutron

Tomoyuki Maruyama, Nobutoshi Yasutake, Myung-Ki Cheoun +3

We make a perturbative calculation of neutrino scattering and absorption in hot and dense hyperonic neutron-star matter in the presence of a strong magnetic Field. We calculate tha…