Efficient numerical solution to vacuum decay with many fields
From MaRDI portal
Publication:5024112
DOI10.1088/1475-7516/2017/01/051OpenAlexW2541654880MaRDI QIDQ5024112
Ali Masoumi, Benjamin Shlaer, Ken D. Olum
Publication date: 28 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1610.06594
Related Items (13)
Vacuum decay and quadratic gravity: the massive case ⋮ Impact of vacuum stability constraints on the phenomenology of supersymmetric models ⋮ Brane nucleation in supersymmetric models ⋮ Detection of early-universe gravitational-wave signatures and fundamental physics ⋮ An optimisation based algorithm for finding the nucleation temperature of cosmological phase transitions ⋮ \texttt{BubbleDet}: a Python package to compute functional determinants for bubble nucleation ⋮ Electroweak baryogenesis and the standard model effective field theory ⋮ Slepian models for Gaussian random landscapes ⋮ Analytic thin wall false vacuum decay rate ⋮ Axion landscape cosmology ⋮ Computing the gauge-invariant bubble nucleation rate in finite temperature effective field theory ⋮ Inflation in multi-field random Gaussian landscapes ⋮ Inflation in random Gaussian landscapes
Uses Software
Cites Work
- Instability of the Kaluza-Klein vacuum
- Bubbles in the supersymmetric standard model
- Tunneling in theories with many fields
- Instability of flat space at finite temperature
- Multiple shooting method for two-point boundary value problems
- THE COSMOLOGICAL CONSTANT PROBLEM AND INFLATION IN THE STRING LANDSCAPE
- A Double Shooting Scheme for Certain Unstable and Singular Boundary Value Problems
- RAPID TUNNELING AND PERCOLATION IN THE LANDSCAPE
- Quantization of four-form fluxes and dynamical neutralization of the cosmological constant
- Unnamed Item
This page was built for publication: Efficient numerical solution to vacuum decay with many fields