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New contribution to WIMP-nucleus scattering
Gary Prézeau, Andriy Kurylov, Marc Kamionkowski +1
A weakly-interacting massive particle (WIMP) is perhaps the most promising candidate for the dark matter in the Galactic halo. The WIMP detection rate in laboratory searches is fix…
What might we learn from a future supernova neutrino signal?
Petr Vogel
Neutrinos from a future Galactic supernova will be detected by several large underground detectors, in particular by SuperKamiokande (SK) and the Sudbury Neutrino Observatory (SNO)…
Can a supernova be located by its neutrinos?
J. F. Beacom, P. Vogel
A future core-collapse supernova in our Galaxy will be detected by several neutrino detectors around the world. The neutrinos escape from the supernova core over several seconds fr…
Neutrino fluence after r-process freeze-out and abundances of Te isotopes in presolar diamonds
Y. -Z. Qian, P. Vogel, G. J. Wasserburg
Using the data of Richter et al. (1998) on Te isotopes in diamond grains from a meteorite, we derive bounds on the neutrino fluence and the decay timescale of the neutrino flux rel…
Supernovae as the Site of the r-Process: Implications for Gamma-Ray Astronomy
Y. -Z. Qian, P. Vogel, G. J. Wasserburg
We discuss how detection of gamma-ray emission from the decay of r-process nuclei can improve our understanding of r-process nucleosynthesis. We find that a gamma-ray detector with…
Diverse Supernova Sources for the r-Process
Y. -Z. Qian, P. Vogel, G. J. Wasserburg
(Abridged) It is shown that a semi-quantitative agreement with the gross solar r-process abundance pattern near and above mass number A=130 can be obtained by a superposition of tw…