Gravitational waves from the vacuum decay with LISA

Abstract

We investigate the gravitational wave spectrum resulted from the cosmological first-order phase transition. We compare two models; one is a scalar field model without gravitation, while the other is a scalar field model with gravitation. Based on the sensitivity curves of the LISA space-based interferometer on the stochastic gravitational-wave background, we compare the difference between the gravitational wave spectra of the former and the latter cases resulted from the bubble collision process. Especially, we calculated the speed of the bubble wall before collision for the two models numerically. We show that the difference between the amplitudes of those spectra can clearly distinguish between the two models. We expect that the LISA with Signal to Noise Ratio =10 could observe the spectrum as the fast first-order phase transition.

References in corpus (60)

• Gravitational Radiation from First-Order Phase Transitions
• Electroweak baryogenesis
• Detecting gravitational waves from cosmological phase transitions with LISA: an update
• The construction and use of LISA sensitivity curves
• Gravitational Wave Production by Collisions: More Bubbles
• Gravitational Radiation from Colliding Vacuum Bubbles: Envelope Approximation to Many-Bubble Collisions
• Science with the space-based interferometer LISA. IV: Probing inflation with gravitational waves
• Cosmological Backgrounds of Gravitational Waves and eLISA/NGO: Phase Transitions, Cosmic Strings and Other Sources
• First-Order Electroweak Phase Transition in the Standard Model with a Low Cutoff
• New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions
• Reconstructing the spectral shape of a stochastic gravitational wave background with LISA
• Primordial black holes and second order gravitational waves from ultra-slow-roll inflation
• The Baryon asymmetry in the Standard Model with a low cut-off
• Detecting a Stochastic Gravitational Wave Background in the presence of a Galactic Foreground and Instrument Noise
• Primordial black holes and gravitational waves from resonant amplification during inflation
• Gravitational waves from bubble dynamics: Beyond the Envelope
• When Primordial Black Holes from Sound Speed Resonance Meet a Stochastic Background of Gravitational Waves
• Cosmological Aspects of Higgs Vacuum Metastability
• Beyond the thin-wall approximation : precise numerical computation of prefactors in false vacuum decay
• The gravitational waves from the first-order phase transition with a dimension-six operator
• Phase transition dynamics and gravitational wave spectra of strong first-order phase transition in supercooled universe
• On bubble collisions in strongly supercooled phase transitions
• The causal structure of dynamical charged black holes
• Is the firewall consistent?: Gedanken experiments on black hole complementarity and firewall proposal
• (Higgs) vacuum decay during inflation
• Determining the outcome of cosmic bubble collisions in full General Relativity
• One-loop corrections to the metastable vacuum decay
• Gravitational waves from first order phase transitions as a probe of an early matter domination era and its inverse problem
• Sound speed resonance of the stochastic gravitational wave background
• Cosmic bubble and domain wall instabilities III: The role of oscillons in three-dimensional bubble collisions
• Mass inflation in f(R) gravity: A conjecture on the resolution of the mass inflation singularity
• Stochastic Gravitational Waves from Inflaton Decays
• Electroweak baryogenesis and gravitational waves in a composite Higgs model with high dimensional fermion representations
• Responses of the Brans-Dicke field due to gravitational collapses
• Constraints on the Reheating Parameters after Gauss-Bonnet Inflation from the Primordial Gravitational Waves
• Simulating the universe(s): from cosmic bubble collisions to cosmological observables with numerical relativity
• Dynamics of false vacuum bubbles: beyond the thin shell approximation
• Beating the Lyth bound by parametric resonance during inflation
• The vacuum bubbles in de Sitter background and black hole pair creation
• Generation of a bubble universe using a negative energy bath
• Bounces with O(3) x O(2) symmetry
• The Thin-Wall Approximation in Vacuum Decay: a Lemma
• Bubble collision with gravitation
• Bubble-nucleation rates for cosmological phase transitions
• Protecting the Stability of the EW Vacuum from Planck-Scale Gravitational Effects
• Black Holes, Oscillating Instantons, and the Hawking-Moss transition
• Instanton solutions mediating tunneling between the degenerate vacua in curved space
• Two-field cosmological phase transitions and gravitational waves in the singlet Majoron model
• Lepton-mediated electroweak baryogenesis, gravitational waves and the $4\tau$ final state at the collider
• Gravitational Wave Spectrum in Inflation with Nonclassical States
• Charged black holes in string-inspired gravity: I. Causal structures and responses of the Brans-Dicke field
• Charged black holes in string-inspired gravity: II. Mass inflation and dependence on parameters and potentials
• Aspects of the negative mode problem in quantum tunneling with gravity
• Coleman-de Luccia instanton in dRGT massive gravity
• Probing new physics with multi-vacua quantum tunnelings beyond standard model through gravitational waves
• Gravitational waves from cosmic bubble collisions
• Black hole factory: a review of double-null formalism
• Moduli destabilization via gravitational collapse
• Cusp singularities in f(R) gravity: pros and cons
• Criteria of existence for bounce solutions in false vacuum decay with gravity

Cited by in corpus (4)

• Prospects for LISA to detect a gravitational-wave background from first order phase transitions
• Reconstructing physical parameters from template gravitational wave spectra at LISA: first order phase transitions
• Gauss-Bonnet Cosmology: large-temperature behaviour and bounds from Gravitational Waves
• Vacuum bubbles from cosmic ripples