Supernova neutrino detection
Publication
, Journal Article
Scholberg, K
Published in: Journal of Physics: Conference Series
January 1, 2012
When a massive star collapses at the end of its life, nearly all of the gravitational binding energy of the resulting remnant is released in the form of neutrinos. The burst of neutrinos from a Galactic core collapse supernova will be detected in neutrino detectors worldwide. This talk will cover supernova neutrino detection techniques in general, current supernova neutrino detectors, and prospects for specific future experiments.
Duke Scholars
Published In
Journal of Physics: Conference Series
DOI
EISSN
1742-6596
ISSN
1742-6588
Publication Date
January 1, 2012
Volume
375
Issue
PART 4
Related Subject Headings
- 0299 Other Physical Sciences
- 0204 Condensed Matter Physics
- 0202 Atomic, Molecular, Nuclear, Particle and Plasma Physics
Citation
APA
Chicago
ICMJE
MLA
NLM
Scholberg, K. (2012). Supernova neutrino detection. Journal of Physics: Conference Series, 375(PART 4). https://doi.org/10.1088/1742-6596/375/1/042036
Scholberg, K. “Supernova neutrino detection.” Journal of Physics: Conference Series 375, no. PART 4 (January 1, 2012). https://doi.org/10.1088/1742-6596/375/1/042036.
Scholberg K. Supernova neutrino detection. Journal of Physics: Conference Series. 2012 Jan 1;375(PART 4).
Scholberg, K. “Supernova neutrino detection.” Journal of Physics: Conference Series, vol. 375, no. PART 4, Jan. 2012. Scopus, doi:10.1088/1742-6596/375/1/042036.
Scholberg K. Supernova neutrino detection. Journal of Physics: Conference Series. 2012 Jan 1;375(PART 4).
Published In
Journal of Physics: Conference Series
DOI
EISSN
1742-6596
ISSN
1742-6588
Publication Date
January 1, 2012
Volume
375
Issue
PART 4
Related Subject Headings
- 0299 Other Physical Sciences
- 0204 Condensed Matter Physics
- 0202 Atomic, Molecular, Nuclear, Particle and Plasma Physics