activity
19932024
most citedNeutrino-Neutrino Scattering and Matter-Enhanced Neutrino Flavor Transformation in Supernovae

185 citations · 843 across the 18 of their papers we have counts for

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15 papers · 1 filter

astro-ph2007★ 98 cited

Flavor Evolution of the Neutronization Neutrino Burst from an O-Ne-Mg Core-Collapse Supernova

Huaiyu Duan, George M. Fuller, J. Carlson +1

We present results of 3-neutrino flavor evolution simulations for the neutronization burst from an O-Ne-Mg core-collapse supernova. We find that nonlinear neutrino self-coupling en…

astro-ph1998★ 107 cited

Prospects for Detecting Supernova Neutrino Flavor Oscillations

G. M. Fuller, W. C. Haxton, G. C. McLaughlin

The neutrinos from a Type II supernova provide perhaps our best opportunity to probe cosmologically interesting muon and/or tauon neutrino masses. This is because matter enhanced n…

astro-ph1996★ 22 cited

Neutrino Gravitational Redshift and the Electron Fraction Above Nascent Neutron Stars

G. M. Fuller, Y. -Z. Qian

Neutrinos emitted from near the surface of the hot proto-neutron star produced by a supernova explosion may be subject to significant gravitational redshift at late times. Electron…

astro-ph1996★ 21 cited

Resonant Neutrino Spin-Flavor Precession and Supernova Nucleosynthesis and Dynamics

H. Nunokawa, Y. -Z. Qian, G. M. Fuller

We discuss the effects of resonant spin-flavor precession (RSFP) of Majorana neutrinos on heavy element nucleosynthesis in neutrino-heated supernova ejecta and the dynamics of supe…

astro-ph1996★ 20 cited

Limits on Active-Sterile Neutrino Mixing and the Primordial Deuterium Abundance

Christian Y. Cardall, George M. Fuller

Studies of limits on active-sterile neutrino mixing derived from big bang nucleosynthesis considerations are extended to consider the dependance of these constraints on the primord…

astro-ph1995★ 75 cited

Matter-enhanced antineutrino flavor transformation and supernova nucleosynthesis

Yong-Zhong Qian, George M. Fuller

Matter-enhanced antineutrino flavor transformation between and can occur in supernovae if the vacuum masses for these species satisfy $m_{\barν_e}>m_{\barν…