Efficient numerical solution to vacuum decay with many fields
read the original abstract
Finding numerical solutions describing bubble nucleation is notoriously difficult in more than one field space dimension. Traditional shooting methods fail because of the extreme non-linearity of field evolution over a macroscopic distance as a function of initial conditions. Minimization methods tend to become either slow or imprecise for larger numbers of fields due to their dependence on the high dimensionality of discretized function spaces. We present a new method for finding solutions which is both very efficient and able to cope with the non-linearities. Our method directly integrates the equations of motion except at a small number of junction points, so we do not need to introduce a discrete domain for our functions. The method, based on multiple shooting, typically finds solutions involving three fields in under a minute, and can find solutions for eight fields in about an hour. We include a numerical package for Mathematica which implements the method described here.
This paper has not been read by Pith yet.
Forward citations
Cited by 3 Pith papers
-
Generalized Virial Identities: Radial Constraints for Solitons, Instantons, and Bounces
A parameterized family of virial identities decomposes global constraints into radially resolved components for O(n)-symmetric solitons, instantons, and bounces.
-
Gauged Q-balls in flat potentials
Gauged Q-balls in flat potentials are qualitatively similar to thin-wall versions, with analytic approximations matching numerics and Proca Q-balls interpolating between global and gauged regimes.
-
TransitionListener v2.0 -- Robust gravitational wave predictions for cosmological phase transitions
TransitionListener v2.0 supplies an end-to-end pipeline from scalar potential to gravitational wave spectra with improved handling of transition dynamics and bubble separation.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.