Published 2009 | Version v1
Miscellaneous Metadata-only

Gravitational waves from core collapse supernovae

Creators

  • 1. Basel University (Switzerland)

Description

Full text: The gravitational wave signal of a core collapse supernova can provide direct observational access to electromagnetically hidden high density regions; it may probe and constrain the nuclear physics properties of the proto-neutron star. We present recent results of 3D simulations of core collapse supernovae performed using different equations of state. The gravitational wave signals from these models will be shown, concentrating on how the signal varies with the equation of state. (author)

Part of:
Nuclear matter at high density. Electronic proceedings of the international workshop 37 on gross properties of nuclei and nuclear excitations

Additional details

Identifiers

URL
http://crunch.ikp.physik.tu-darmstadt.de/nhc/pages/events/hirschegg/2009/listofabstracts2.php; http://crunch.ikp.physik.tu-darmstadt.de/nhc/pages/events/hirschegg/2009/talks/Proceedings/Scheidegger.pdf;

Publishing Information

Imprint Place
Darmstadt (Germany)
Imprint Title
Nuclear matter at high density. Electronic proceedings of the international workshop 37 on gross properties of nuclei and nuclear excitations
Imprint Pagination
[200 p.]
Journal Page Range
[1 p.]

Conference

Title
International workshop 37 on gross properties of nuclei and nuclear excitations
Acronym
Nuclear matter at high density
Dates
18-24 Jan 2009
Place
Hirschegg (Austria)

INIS

Country of Publication
Germany
Country of Input or Organization
Austria
INIS RN
41095222
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference, Non-conventional Literature
Descriptors DEI
COMPUTERIZED SIMULATION; EQUATIONS OF STATE; GRAVITATIONAL WAVES; SUPERNOVAE; THREE-DIMENSIONAL CALCULATIONS
Descriptors DEC
BINARY STARS; EQUATIONS; ERUPTIVE VARIABLE STARS; SIMULATION; STARS; VARIABLE STARS

Optional Information