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Detecting gravitational waves from cosmological phase transitions with LISA: an update
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…
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The next-generation liquid-scintillator neutrino observatory LENA
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Generic rules for high temperature dimensional reduction and their application to the Standard Model
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RESONANCE SCATTERING PHASE SHIFTS ON A NON-REST FRAME LATTICE
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Shape of the acoustic gravitational wave power spectrum from a first order phase transition
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…
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Numerical simulations of acoustically generated gravitational waves at a first order phase transition
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…
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Sphaleron rate in the minimal standard model.
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…
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3D physics and the electroweak phase transition: Perturbation theory and lattice Monte Carlo analysis
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The Pressure of hot QCD up to g6 ln(1/g)
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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The Electroweak Phase Transition: A Non-Perturbative Analysis
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