Published August 15, 1995 | Version v1
Journal article

Oscillons: Resonant configurations during bubble collapse

  • 1. School of Mathematical and Physical Sciences, University of Sussex, Brighton BN1 9QH (United Kingdom)
  • 2. NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510 (United States)
  • 3. Department of Physics and Astronomy, Dartmouth College, Hanover, New Hampshire 03755 (United States)

Description

Oscillons are localized, nonsingular, time-dependent, spherically symmetric solutions of nonlinear scalar field theories which, although unstable, are extremely long lived. We show that they naturally appear during the collapse of subcritical bubbles in models with symmetric and asymmetric double-well potentials. By a combination of analytical and numerical work we explain several of their properties, including the conditions for their existence, their longevity, and their final demise. We discuss several contexts in which we expect oscillons to be relevant. In particular, their nucleation during cosmological phase transitions may have wide-ranging consequences

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
52
Journal Issue
4
Journal Page Range
p. 1920-1933.
ISSN
0556-2821
CODEN
PRVDAQ

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
27020560
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Descriptors DEI
BUBBLES; COSMOLOGY; NONLINEAR PROBLEMS; NUCLEATION; PHASE TRANSFORMATIONS; SCALAR FIELDS; TIME DEPENDENCE