Impact of theoretical uncertainties on model parameter reconstruction from GW signals sourced by cosmological phase transitions
Different computational techniques for cosmological phase transition parameters can impact
the gravitational wave (GW) spectra predicted in a given particle physics model. To …
the gravitational wave (GW) spectra predicted in a given particle physics model. To …
Black Holes and Gravitational Waves from Slow First-Order Phase Transitions
Slow first-order phase transitions generate large inhomogeneities that can lead to the
formation of primordial black holes. We show that the gravitational wave spectrum then …
formation of primordial black holes. We show that the gravitational wave spectrum then …
Triple Higgs boson production and electroweak phase transition in the two-real-singlet model
O Karkout, A Papaefstathiou, M Postma… - Journal of High Energy …, 2024 - Springer
A bstract The production of three Higgs bosons at hadron colliders can be enhanced by a
double-resonant effect in the ℤ 2-symmetric two-real-singlet extension of the Standard …
double-resonant effect in the ℤ 2-symmetric two-real-singlet extension of the Standard …
Primordial gravitational wave backgrounds from phase transitions with next generation ground based detectors
C Caprini, O Pujolàs… - … and Quantum Gravity, 2025 - iopscience.iop.org
Primordial gravitational wave backgrounds from phase transitions with next generation
ground based detectors - IOPscience Skip to content IOP Science home Accessibility Help …
ground based detectors - IOPscience Skip to content IOP Science home Accessibility Help …
Hot new early dark energy bridging cosmic gaps: Supercooled phase transition reconciles stepped dark radiation solutions to the Hubble tension with BBN
We propose a simple model that can alleviate the H 0 tension while remaining consistent
with big bang nucleosynthesis (BBN). It is based on a dark sector described by a standard …
with big bang nucleosynthesis (BBN). It is based on a dark sector described by a standard …
Slaying axion-like particles via gravitational waves and primordial black holes from supercooled phase transition
A bstract We study the formation of primordial black holes (PBHs) from density fluctuations
due to supercooled phase transitions (PTs) triggered in an axion-like particle (ALP) model …
due to supercooled phase transitions (PTs) triggered in an axion-like particle (ALP) model …
How fast does the WallGo? A package for computing wall velocities in first-order phase transitions
A Ekstedt, O Gould, J Hirvonen, B Laurent… - arxiv preprint arxiv …, 2024 - arxiv.org
WallGo is an open source software for the computation of the bubble wall velocity in first-
order cosmological phase transitions. It also computes the energy budget available for the …
order cosmological phase transitions. It also computes the energy budget available for the …
Refining Gravitational wave and collider physics dialogue via singlet scalar extension
MJ Ramsey-Musolf, TVI Tenkanen, VQ Tran - arxiv preprint arxiv …, 2024 - arxiv.org
Employing effective field theory techniques, we advance computations of thermal
parameters that enter predictions for the gravitational wave spectra from first-order …
parameters that enter predictions for the gravitational wave spectra from first-order …
[HTML][HTML] Radiative symmetry breaking from the on-shell perspective
B Sójka, B Świeżewska - Physics Letters B, 2025 - Elsevier
Abstract Models with classical scale symmetry, which feature radiative symmetry breaking,
generically lead to a supercooled first-order phase transition in the early Universe resulting …
generically lead to a supercooled first-order phase transition in the early Universe resulting …
Bubble-wall speed with loop corrections
A Dashko, A Ekstedt - arxiv preprint arxiv:2411.05075, 2024 - arxiv.org
In this paper, we investigate the dynamics of the nucleating scalar field during the first-order
phase transitions by incorporating one-loop corrections of classical fluctuations. We assume …
phase transitions by incorporating one-loop corrections of classical fluctuations. We assume …