activity
20152026
most citedAEDGE: Atomic Experiment for Dark Matter and Gravity Exploration in Space

365 citations · 5.2k across the 57 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

35 papers · 1 filter

astro-ph.CO2026

Benchmarking wall velocities in cosmological phase transitions: Fluid Ansatz and WallGo

Gláuber C. Dorsch, Marek Lewicki, Daniel A. Pinto

A reliable computation of the bubble wall velocity during a cosmological phase transition requires an adequate modeling of the non-equilibrium dynamics in the vicinity of this expa…

astro-ph.CO2026

From friction scaling to an efficient method for estimating bubble wall velocity

Tomasz Krajewski, Marek Lewicki, Marco Merchand +2

We present a unified description of first-order cosmological phase transition dynamics that links the phenomenological friction model employed in hydrodynamic simulations to the mi…

astro-ph.CO2025

Impact of cosmic expansion on gravitational wave spectra from strongly supercooled first-order phase transitions

Marek Lewicki, Ville Vaskonen

We compute the gravitational wave spectra from strongly supercooled first-order phase transitions, explicitly incorporating the evolution of the background metric across the transi…

astro-ph.CO2024★ 13 cited

Black holes and gravitational waves from phase transitions in realistic models

Marek Lewicki, Piotr Toczek, Ville Vaskonen

We study realistic models predicting primordial black hole (PBH) formation from density fluctuations generated in a first-order phase transition. We show that the second-order corr…

astro-ph.CO2024★ 6 cited

Steady-state bubbles beyond local thermal equilibrium

Tomasz Krajewski, Marek Lewicki, Ignacy Nałęcz +1

We investigate the hydrodynamic solutions for expanding bubbles in cosmological first-order phase transitions going beyond local thermal equilibrium approximation. Under the assump…

astro-ph.CO2024★ 4 cited

Gravitational waves from cosmic strings in LISA: reconstruction pipeline and physics interpretation

Jose J. Blanco-Pillado, Yanou Cui, Sachiko Kuroyanagi +6

We initiate the LISA template databank for stochastic gravitational wave backgrounds sourced by cosmic strings. We include two templates, an analytical template, which enables more…

astro-ph.CO2024★ 72 cited

Gravitational waves from first-order phase transitions in LISA: reconstruction pipeline and physics interpretation

Chiara Caprini, Ryusuke Jinno, Marek Lewicki +6

We develop a tool for the analysis of stochastic gravitational wave backgrounds from cosmological first-order phase transitions with LISA: we initiate a template databank for these…

astro-ph.CO2024★ 45 cited

LISA Definition Study Report

Monica Colpi, Karsten Danzmann, Martin Hewitson +108

The Laser Interferometer Space Antenna (LISA) is the first scientific endeavour to detect and study gravitational waves from space. LISA will survey the sky for Gravitational Waves…

astro-ph.CO2024★ 28 cited

Bubble-wall velocity in local thermal equilibrium: hydrodynamical simulations vs analytical treatment

Tomasz Krajewski, Marek Lewicki, Mateusz Zych

We perform real-time hydrodynamical simulations of the growth of bubbles formed during cosmological first-order phase transitions under the assumption of local thermal equilibrium.…

astro-ph.CO2024

Black holes and gravitational waves from slow phase transitions

Marek Lewicki, Piotr Toczek, Ville Vaskonen

Slow first-order phase transitions generate large inhomogeneities that can lead to the formation of primordial black holes (PBHs). We show that the gravitational wave (GW) spectrum…

astro-ph.CO2023★ 8 cited

From Hubble to Bubble

Maciej Kierkla, Giorgio Laverda, Marek Lewicki +4

The detection of a stochastic Gravitational Wave (GW) background sourced by a cosmological phase transition would allow us to see the early Universe from a completely new perspecti…

astro-ph.CO2023★ 1 cited

What is the source of the PTA GW signal?

John Ellis, Malcolm Fairbairn, Gabriele Franciolini +7

The most conservative interpretation of the nHz stochastic gravitational wave background (SGWB) discovered by NANOGrav and other Pulsar Timing Array (PTA) Collaborations is astroph…

astro-ph.CO2023★ 8 cited

Cosmic Superstrings Revisited in Light of NANOGrav 15-Year Data

John Ellis, Marek Lewicki, Chunshan Lin +1

We analyze cosmic superstring models in light of NANOGrav 15-year pulsar timing data. A good fit is found for a string tension and a string intercommu…

astro-ph.CO2023★ 106 cited

Primordial black holes from strong first-order phase transitions

Marek Lewicki, Piotr Toczek, Ville Vaskonen

We study the formation of primordial black holes (PBHs) in strongly supercooled first-order phase transitions. The mechanism is based on the presence of remnants dominated by the f…

astro-ph.CO2023

Imprints of a Supercooled Phase Transition in the Gravitational Wave Spectrum from a Cosmic String network

Francesc Ferrer, Anish Ghoshal, Marek Lewicki

A network of cosmic strings (CS), if present, would continue emitting gravitational waves (GW) as it evolves throughout the history of the Universe. This results in a characteristi…

astro-ph.CO2023★ 27 cited

Hydrodynamical constraints on bubble wall velocity

Tomasz Krajewski, Marek Lewicki, Mateusz Zych

Terminal velocity reached by bubble walls in first order phase transitions is an important parameter determining both primordial gravitational-wave spectrum and production of baryo…

astro-ph.CO2022★ 54 cited

Distinct signatures of spinning PBH domination and evaporation: doubly peaked gravitational waves, dark relics and CMB complementarity

Nilanjandev Bhaumik, Anish Ghoshal, Rajeev Kumar Jain +1

Ultra-low mass primordial black holes (PBH), which may briefly dominate the energy density of the universe but completely evaporate before the big bang nucleosynthesis (BBN), can l…

astro-ph.CO2022★ 92 cited

Gravitational waves from bubble collisions and fluid motion in strongly supercooled phase transitions

Marek Lewicki, Ville Vaskonen

We estimate the gravitational wave spectra generated in strongly supercooled phase transitions by bubble collisions and fluid motion. We derive analytically in the thin-wall approx…

astro-ph.CO2022★ 76 cited

Doubly peaked induced stochastic gravitational wave background : Testing baryogenesis from primordial black holes

Nilanjandev Bhaumik, Anish Ghoshal, Marek Lewicki

Hawking evaporation of primordial black holes (PBHs) can facilitate the generation of matter-antimatter asymmetry. We focus on ultra-low mass PBHs that briefly dominate the univers…

astro-ph.CO2022★ 21 cited

Bubble dynamics in fluids with N-body simulations

Marek Lewicki, Ville Vaskonen, Hardi Veermäe

We present a new approach to studies of bubble dynamics in fluids. Relying on particle-based simulations, this method is general and suitable for cases where the commonly used perf…

astro-ph.CO2022★ 359 cited

Cosmology with the Laser Interferometer Space Antenna

Pierre Auclair, David Bacon, Tessa Baker +177

The Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological focus: to probe the expansion rate of the universe, and to understand stochastic gravita…

astro-ph.CO2021★ 99 cited

Electroweak bubble wall expansion: gravitational waves and baryogenesis in Standard Model-like thermal plasma

Marek Lewicki, Marco Merchand, Mateusz Zych

Computing the properties of the bubble wall of a cosmological first order phase transition at electroweak scale is of paramount importance for the correct prediction of the baryon…

astro-ph.CO2021★ 20 cited

Impact of LIGO-Virgo black hole binaries on gravitational wave background searches

Marek Lewicki, Ville Vaskonen

We study the impact of the black hole binary population currently probed by LIGO-Virgo on future searches for the primordial gravitational wave background. We estimate the foregrou…

astro-ph.CO2021★ 39 cited

Escape from supercooling with or without bubbles: gravitational wave signatures

Marek Lewicki, Oriol Pujolàs, Ville Vaskonen

Quasi-conformal models are an appealing scenario that can offer naturally a strongly supercooled phase transition and a period of thermal inflation in the early Universe. A crucial…