Published October 15, 2001 | Version v1
Journal article

Quenching processes in flame-vortex interactions

  • 1. Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637 (United States)
  • 2. Center for Astrophysical Thermonuclear Flashes, Chicago, Illinois 60637 (United States)
  • 3. Max-Planck-Institut fuer Astrophysik, Garching, Germany 85748 (Germany)
  • 4. Goddard Space Flight Center, Greenbelt, Maryland 20771 (United States)

Description

We show direct numerical simulations of flame-vortex interactions in order to understand quenching of thermonuclear flames. The key question is--can a thermonuclear flame be quenched? If not, the deflagration-detonation transition mechanisms that demand a finely tuned preconditioned region in the interior of a white dwarf are unlikely to work. In these simulations, we pass a steady-state laminar flame through a vortex pair. The vortex pair represents the most severe strain the flame front will encounter inside the white dwarf. We perform a parameter study, varying the speed and size of the vortex pair, in order to understand the quenching process. No quenching is observed in any of the calculations performed to date

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
586
Journal Issue
1
Journal Page Range
p. 490-492
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
20. Texas symposium on relativistic astrophysics
Dates
10-15 Dec 2000
Place
Austin, TX (United States)

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
35076204
Subject category
S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
COMPUTERIZED SIMULATION; FLAMES; LAMINAR FLOW; NUMERICAL ANALYSIS; QUENCHING; SUPERNOVAE; THERMONUCLEAR EXPLOSIONS; VORTICES
Descriptors DEC
BINARY STARS; ERUPTIVE VARIABLE STARS; EXPLOSIONS; FLUID FLOW; MATHEMATICS; NUCLEAR EXPLOSIONS; SIMULATION; STARS; VARIABLE STARS

Optional Information

Notes
(c) 2001 American Institute of Physics.