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CERN Document Server Encontrados 7 registros  La búsqueda tardó 0.53 segundos. 
1.
Bounds on the bubble wall velocity / Ai, Wen-Yuan (King's Coll. London) ; Laurent, Benoit (McGill U., Montreal (main)) ; van de Vis, Jorinde (CERN)
Determining the bubble wall velocity in first-order phase transitions is a challenging task, requiring the solution of (coupled) equations of motion for the scalar field and Boltzmann equations for the particles in the plasma. [...]
CERN-TH-2024-198 ; KCL-PH-TH/2024-57 ; arXiv:2411.13641. - 47.
Fulltext
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2.
How fast does the WallGo? A package for computing wall velocities in first-order phase transitions / Ekstedt, Andreas (Uppsala U. (main)) ; Gould, Oliver (U. Nottingham) ; Hirvonen, Joonas (U. Nottingham ; Helsinki Inst. of Phys. ; U. Helsinki (main)) ; Laurent, Benoit (McGill U., Montreal (main)) ; Niemi, Lauri (Helsinki Inst. of Phys. ; U. Helsinki (main)) ; Schicho, Philipp (U. Geneva (main)) ; van de Vis, Jorinde (CERN)
WallGo is an open source software for the computation of the bubble wall velocity in first-order cosmological phase transitions. [...]
CERN-TH-2024-174 ; DESY-24-162 ; HIP-2024-21/TH ; arXiv:2411.04970. - 71.
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Stochastic gravitational waves from cosmological phase transitions / van de Vis, Jorinde (speaker)
2023 - 1815. Eucapt Conferences; Third EuCAPT Annual Symposium External links: Talk details; Event details In : Third EuCAPT Annual Symposium
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4.
Cosmology with the Laser Interferometer Space Antenna / LISA Cosmology Working Group Collaboration
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 gravitational-wave backgrounds and their implications for early universe and particle physics, from the MeV to the Planck scale. However, the range of potential cosmological applications of gravitational wave observations extends well beyond these two objectives. [...]
arXiv:2204.05434; LISA CosWG-22-03; FERMILAB-PUB-22-349-SCD.- 2023-08-28 - 176 p. - Published in : Living Rev. Relativ. 26 (2023) 5 Fulltext: jt - PDF; 2204.05434 - PDF; Fulltext from Publisher: PDF; External link: Fermilab Library Server
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5.
Early-Universe Model Building / Asadi, Pouya (MIT, Cambridge, CTP) ; Bansal, Saurabh (Cincinnati U.) ; Berlin, Asher (Fermilab ; New York U.) ; Co, Raymond T. (Minnesota U., Theor. Phys. Inst.) ; Croon, Djuna (Durham U., IPPP) ; Cui, Yanou (UC, Riverside) ; Curtin, David (Toronto U.) ; Cyr-Racine, Francis-Yan (New Mexico U.) ; Davoudiasl, Hooman (BNL, NSLS) ; Rose, Luigi Delle (Barcelona, IFAE ; BIST, Barcelona) et al.
Theoretical investigations into the evolution of the early universe are an essential part of particle physics that allow us to identify viable extensions to the Standard Model as well as motivated parameter space that can be probed by various experiments and observations. [...]
arXiv:2203.06680 ; FERMILAB-CONF-22-158-T. - 206 p.
Fermilab Library Server - eConf - Fulltext - Fulltext
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6.
New Ideas in Baryogenesis: A Snowmass White Paper / Elor, Gilly (U. Mainz, PRISMA ; Mainz U.) ; Harz, Julia (Munich, Tech. U.) ; Ipek, Seyda (Carleton U.) ; Shakya, Bibhushan (DESY) ; Blinov, Nikita (Victoria U.) ; Co, Raymond T. (Minnesota U., Theor. Phys. Inst.) ; Cui, Yanou (UC, Riverside) ; Dasgupta, Arnab (Brookhaven) ; Davoudiasl, Hooman (Pittsburgh U.) ; Elahi, Fatemeh (U. Mainz, PRISMA ; Mainz U.) et al.
The Standard Model of Particle Physics cannot explain the observed baryon asymmetry of the Universe. [...]
arXiv:2203.05010. -
eConf - Fulltext
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7.
Model-independent energy budget for LISA / Giese, Felix (DESY) ; Konstandin, Thomas (DESY) ; Schmitz, Kai (CERN) ; van de Vis, Jorinde (DESY)
We provide an easy method to obtain the kinetic energy fraction in gravitational waves, generated during a cosmological first-order phase transition, as a function of only the wall velocity and quantities that can be determined from the particle physics model at the nucleation temperature. This generalizes recent work that achieved this goal for detonations. [...]
arXiv:2010.09744; DESY-20-173; DESY 20-173; CERN-TH-2020-170.- 2021-01-29 - 31 p. - Published in : JCAP 2101 (2021) 072 Fulltext: PDF;
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