Ando, Shin'ichiro (2007) Neutrino Probes of Galactic and Extragalactic Supernovae. In: Tours Symposium on Nuclear Physics VI. AIP Conference Proceedings (891). American Institute of Physics , Melville, NY, pp. 263-271. ISBN 978-0-7354-0395-6 http://resolver.caltech.edu/CaltechAUTHORS:20100819-111653720
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Neutrinos are a messenger of extreme condition inside a supernova core and a new-born neutron star. Since current ground-based detectors have potential to detect ~10,000 neutrinos from supernova at the galactic center, they could tell us lots of important physics. It includes: explosion mechanism, shock wave propagation, core temperature, and gravitational binding energy, as well as neutrino properties as elementary particle. In addition to the galactic supernova neutrino burst, one can still learn about them with diffuse supernova neutrino background, which is also soon to be detected. We review current situation from both points of view, and discuss prospects for future neutrino astrophysics.
|Item Type:||Book Section|
|Additional Information:||© 2007 American Institute of Physics. The author acknowledges support from Sherman Fairchild Foundation at Caltech.|
|Subject Keywords:||supernovae; neutrinos; diffuse background; elementary particle physics|
|Classification Code:||PACS: 95.55.Vj; 95.85.Ry; 97.60.Bw|
|Official Citation:||Neutrino Probes of Galactic and Extragalactic Supernovae Shin'ichiro Ando, AIP Conf. Proc. 891, 263 (2007), DOI:10.1063/1.2713526|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Tony Diaz|
|Deposited On:||20 Aug 2010 20:51|
|Last Modified:||26 Dec 2012 12:20|
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