Published 1981 | Version v1
Report Restricted

Research in nuclear astrophysics: stellar collapse and supernovae. Progress report, December 1, 1981-November 30, 1984

Creators

Description

The implications of nuclear theory for the final collapse of massive stars will be examined. Development of an appropriate nuclear equation of state and its implementation in hydrodynamic studies will be continued. The influence of nuclear dissociation and neutrino emission on the formation and propagation of shocks will be studied. The long term evolution of collapsed stellar cores after the initial hydrodynamic bounce will be investigated. Neutrino production and emission in all phases will be derived. Potential effects of pion condensation and neutrino instabilities will be explored

Availability note (English)

MF available from INIS under the Report Number; Available from NTIS., PC A03/MF A01.

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Additional details

Publishing Information

Imprint Pagination
40 p.
Report number
DOE/ER/10719--T1

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
13646330
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Progress Report
Descriptors DEI
HYDRODYNAMIC MODEL; NUCLEAR PHYSICS; SHOCK WAVES; STAR EVOLUTION; SUPERNOVAE; WAVE PROPAGATION
Descriptors DEC
ERUPTIVE VARIABLE STARS; MATHEMATICAL MODELS; PARTICLE MODELS; PHYSICS; STARS; STATISTICAL MODELS; THERMODYNAMIC MODEL; VARIABLE STARS