Supernova neutrino detection
Publication
, Journal Article
Scholberg, K
Published in: Nuclear Physics B - Proceedings Supplements
January 1, 2001
World-wide, several detectors currently running or neaxing completion are sensitive to a core collapse supernova neutrino signal in the Galaxy. I will briefly describe the nature of the neutrino signal and then survey current and future detection techniques. I will also explore what physics and astrophysics we can learn from the next Galactic core collapse.
Duke Scholars
Published In
Nuclear Physics B - Proceedings Supplements
DOI
ISSN
0920-5632
Publication Date
January 1, 2001
Volume
91
Issue
1-3
Start / End Page
331 / 337
Citation
APA
Chicago
ICMJE
MLA
NLM
Scholberg, K. (2001). Supernova neutrino detection. Nuclear Physics B - Proceedings Supplements, 91(1–3), 331–337. https://doi.org/10.1016/s0920-5632(00)00959-2
Scholberg, K. “Supernova neutrino detection.” Nuclear Physics B - Proceedings Supplements 91, no. 1–3 (January 1, 2001): 331–37. https://doi.org/10.1016/s0920-5632(00)00959-2.
Scholberg K. Supernova neutrino detection. Nuclear Physics B - Proceedings Supplements. 2001 Jan 1;91(1–3):331–7.
Scholberg, K. “Supernova neutrino detection.” Nuclear Physics B - Proceedings Supplements, vol. 91, no. 1–3, Jan. 2001, pp. 331–37. Scopus, doi:10.1016/s0920-5632(00)00959-2.
Scholberg K. Supernova neutrino detection. Nuclear Physics B - Proceedings Supplements. 2001 Jan 1;91(1–3):331–337.
Published In
Nuclear Physics B - Proceedings Supplements
DOI
ISSN
0920-5632
Publication Date
January 1, 2001
Volume
91
Issue
1-3
Start / End Page
331 / 337