Published October 1, 2006
| Version v1
Journal article
Damping of neutrino flavour conversions in a 'noisy' supernova shock-wave
Creators
- 1. Dipartimento di Fisica and Sezione INFN di Bari, Via Amendola 173, 70126 Bari (Italy)
- 2. Dipartimento di Fisica and Sezione INFN di Lecce, Via Arnesano, 73100 Lecce (Italy)
Description
In recent literature, it has been realized that supernova (SN) shock-wave propagation after the core-bounce can leave a peculiar imprint on the observable SN neutrino signal at Earth. We show that small-scale stochastic density fluctuations in SN matter might modify this scenario, potentially suppressing the signature associated with the shock wave on the neutrino spectra
Availability note (English)
Available online at http://stacks.iop.org/1402-4896/T127/80/physscr6_T127_028.pdf or at the Web site for the journal Physica Scripta (Online) (ISSN 1402-4896) http://www.iop.org/Additional details
Identifiers
- URL
- http://stacks.iop.org/1402-4896/T127/80/physscr6_T127_028.pdf; http://www.iop.org/;
- DOI
- 10.1088/0031-8949/2006/T127/028;
- PII
- S0031-8949(06)28342-28;
Publishing Information
- Journal Title
- Physica Scripta (Online)
- Journal Volume
- 2006
- Journal Issue
- T127
- Journal Page Range
- p. 80-81
- ISSN
- 1402-4896
Conference
- Title
- 2. Scandanavian Neutrino Workshop (SNOW 2006)
- Dates
- 2-6 May 2006
- Place
- Stockholm (Sweden)
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38003664
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- DENSITY; FLAVOR MODEL; NEUTRINOS; SHOCK WAVES; STOCHASTIC PROCESSES; SUPERNOVAE; WAVE PROPAGATION
- Descriptors DEC
- BINARY STARS; COMPOSITE MODELS; ELEMENTARY PARTICLES; ERUPTIVE VARIABLE STARS; FERMIONS; LEPTONS; MASSLESS PARTICLES; MATHEMATICAL MODELS; PARTICLE MODELS; PHYSICAL PROPERTIES; QUARK MODEL; STARS; VARIABLE STARS