Running with Constant Energy

@inproceedings{Franois1994RunningWC,
  title={Running with Constant Energy},
  author={C. François and Christophe Samson},
  booktitle={ICRA},
  year={1994}
}
Overview • Renormalisation group running vacuum energy exchanging energy-momentum with neutrinos. • Eective interaction between the cosmological constant (CC) and cosmic relic neutrinos. • Relic neutrino distribution function modied non-trivial properties. • CC time-dependent background evolution modied. • Phenomenological implications: neutrino mass bounds, freestreaming. 

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@BULLET Massive quantum elds: RG running vacuum energy. Energy-momentum transfer

@BULLET Massive quantum elds: RG running vacuum energy. Energy-momentum transfer

@BULLET arxiv: 0711

@BULLET arxiv: 0711

@BULLET ν: Energy density and average momentum reduced highly degenerated distribution function

@BULLET ν: Energy density and average momentum reduced highly degenerated distribution function

Eective interaction with matter/particles

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Relaxed (cosmological) bounds on m ν . Modied freestreaming signatures

Relaxed (cosmological) bounds on m ν . Modied freestreaming signatures

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