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Detecting gravitational waves from cosmological phase transitions with LISA: an update
- C. Caprini, M. Chala, D. Weir
- PhysicsJournal of Cosmology and Astroparticle Physics
- 29 October 2019
We investigate the potential for observing gravitational waves from cosmological phase transitions with LISA in light of recent theoretical and experimental developments. Our analysis is based on…
Generic rules for high temperature dimensional reduction and their application to the Standard Model
- K. Kajantie, M. Laine, K. Rummukainen, M. Shaposhnikov
- Physics
- 1996
RESONANCE SCATTERING PHASE SHIFTS ON A NON-REST FRAME LATTICE
- K. Rummukainen, S. Gottlieb
- Physics
- 31 March 1995
Shape of the acoustic gravitational wave power spectrum from a first order phase transition
- M. Hindmarsh, S. Huber, K. Rummukainen, D. Weir
- Physics
- 19 April 2017
We present results from large-scale numerical simulations of a first order thermal phase transition in the early Universe, in order to explore the shape of the acoustic gravitational wave and the…
Numerical simulations of acoustically generated gravitational waves at a first order phase transition
- M. Hindmarsh, S. Huber, K. Rummukainen, D. Weir
- Physics
- 13 April 2015
We present details of numerical simulations of the gravitational radiation produced by a first order thermal phase transition in the early universe. We confirm that the dominant source of…
Sphaleron rate in the minimal standard model.
- M. D’Onofrio, K. Rummukainen, A. Tranberg
- PhysicsPhysical review letters
- 14 April 2014
We use large-scale lattice simulations to compute the rate of baryon number violating processes (the sphaleron rate), the Higgs field expectation value, and the critical temperature in the standard…
3D physics and the electroweak phase transition: Perturbation theory and lattice Monte Carlo analysis
- K. Farakos, K. Kajantie, K. Rummukainen, M. Shaposhnikov
- Physics
- 1 April 1994
The Pressure of hot QCD up to g6 ln(1/g)
- K. Kajantie, M. Laine, K. Rummukainen, Y. Schroder
- Physics
- 20 November 2002
The free energy density, or pressure, of QCD has at high temperatures an expansion in the coupling constant g, known so far up to order g^5. We compute here the last contribution which can be…
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