0000000000891219

AUTHOR

Stephan J. Huber

showing 2 related works from this author

A Tachyonic Gluon Mass: Between Infrared and Ultraviolet

1999

The gluon spin coupling to a Gaussian correlated background gauge field induces an effective tachyonic gluon mass. It is momentum dependent and vanishes in the UV only like 1/p^2. In the IR, we obtain stabilization through a positive m^2_{conf}(p^2) related to confinement. Recently a purely phenomenological tachyonic gluon mass was used to explain the linear rise in the q\bar q static potential at small distances and also some long standing discrepancies found in QCD sum rules. We show that the stochastic vacuum model of QCD predicts a gluon mass with the desired properties.

Quantum chromodynamicsPhysicsNuclear and High Energy PhysicsQCD sum rulesParticle physicsStochastic vacuum modelHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyFOS: Physical sciencesCoupling (probability)GluonMomentumHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics::ExperimentGauge theorySpin-½
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Detecting gravitational waves from cosmological phase transitions with LISA: an update

2020

MC was funded by the Royal Society under the Newton International Fellowship program. GD would like to thank CNPq (Brazil) for financial support. MH was supported by the Science and Technology Facilities Council (grant number ST/P000819/1), and the Academy of Finland (grant number 286769). SJH was supported by the Science and Technology Facilities Council (grant number ST/P000819/1). The work of JK was supported by Department of Energy (DOE) grant DE-SC0019195 and NSF grant PHY-1719642. TK and GS are funded by the Deutsche Forschungsgemeinschaft under Germany's Excellence Strategy - EXC 2121 \Quantum Universe" - 390833306. JMN is supported by Ramon y Cajal Fellowship contract RYC-2017-22986…

Phase transitionCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard ModelDark matterstandard modelFOS: Physical sciencesContext (language use)gravitational radiation: direct detection01 natural sciencesdark matterbubble: nucleationGravitational wavesTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)effective field theory0103 physical sciencesEffective field theoryenergy: densitynumerical calculationsCosmological phase transitionsperturbation theoryPhysics:Matematikk og Naturvitenskap: 400::Fysikk: 430 [VDP]wave: acousticLISACOSMIC cancer database010308 nuclear & particles physicsGravitational wavenew physicsGravitational theorygravitational radiationAstronomy and Astrophysicscritical phenomenagravitational radiation detectorHigh Energy Physics - PhenomenologyGravitational sourcesgravitational radiation: emission[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Higgs modelPerturbation theory (quantum mechanics)gravitational radiation: power spectrum[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]dilatonAstrophysics - Cosmology and Nongalactic Astrophysics
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