Supernova neutrino detection
Publication
, Journal Article
Scholberg, K
Published in: Nuclear Physics B - Proceedings Supplements
December 1, 2011
The gravitational core collapse of a star produces a huge burst of neutrinos of all flavors. A number of detectors worldwide are sensitive to such a burst; its detection would yield information about both particle physics and astrophysics. Sensitivity to all flavors, and ability to tag different interactions will be key for extraction of information. Here I will survey the capabilities of current and future detectors for detection of supernova neutrinos from the Milky Way and beyond. © 2011 Elsevier B.V.
Duke Scholars
Published In
Nuclear Physics B - Proceedings Supplements
DOI
ISSN
0920-5632
Publication Date
December 1, 2011
Volume
221
Start / End Page
248 / 253
Citation
APA
Chicago
ICMJE
MLA
NLM
Scholberg, K. (2011). Supernova neutrino detection. Nuclear Physics B - Proceedings Supplements, 221, 248–253. https://doi.org/10.1016/j.nuclphysbps.2011.09.012
Scholberg, K. “Supernova neutrino detection.” Nuclear Physics B - Proceedings Supplements 221 (December 1, 2011): 248–53. https://doi.org/10.1016/j.nuclphysbps.2011.09.012.
Scholberg K. Supernova neutrino detection. Nuclear Physics B - Proceedings Supplements. 2011 Dec 1;221:248–53.
Scholberg, K. “Supernova neutrino detection.” Nuclear Physics B - Proceedings Supplements, vol. 221, Dec. 2011, pp. 248–53. Scopus, doi:10.1016/j.nuclphysbps.2011.09.012.
Scholberg K. Supernova neutrino detection. Nuclear Physics B - Proceedings Supplements. 2011 Dec 1;221:248–253.
Published In
Nuclear Physics B - Proceedings Supplements
DOI
ISSN
0920-5632
Publication Date
December 1, 2011
Volume
221
Start / End Page
248 / 253