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Title: Probing nonstandard decoherence effects with solar and KamLAND neutrinos

Journal Article · · Physical Review. D, Particles Fields
; ;  [1];  [2];  [1]
  1. Dipartimento di Fisica and Sezione INFN di Bari, Via Amendola 173, 70126, Bari (Italy)
  2. Dipartimento di Fisica and Sezione INFN di Lecce, Via Arnesano, 73100 Lecce (Italy)

It has been speculated that quantum-gravity might induce a foamy space-time structure at small scales, randomly perturbing the propagation phases of free-streaming particles (such as kaons, neutrons, or neutrinos). Particle interferometry might then reveal nonstandard decoherence effects, in addition to standard ones (due to, e.g., finite source size and detector resolution.) In this work we discuss the phenomenology of such nonstandard effects in the propagation of electron neutrinos in the Sun and in the long-baseline reactor experiment KamLAND, which jointly provide us with the best available probes of decoherence at neutrino energies E{approx}few MeV. In the solar neutrino case, by means of a perturbative approach, decoherence is shown to modify the standard (adiabatic) propagation in matter through a calculable damping factor. By assuming a power-law dependence of decoherence effects in the energy domain (E{sup n} with n=0, {+-}1, {+-}2), theoretical predictions for two-family neutrino mixing are compared with the data and discussed. We find that neither solar nor KamLAND data show evidence in favor of nonstandard decoherence effects, whose characteristic parameter {gamma}{sub 0} can thus be significantly constrained. In the ''Lorentz-invariant'' case n=-1, we obtain the upper limit {gamma}{sub 0}<0.78x10{sup -26} GeV at 95% C.L. In the specific case n=-2, the constraints can also be interpreted as bounds on possible matter density fluctuations in the Sun, which we improve by a factor of {approx}2 with respect to previous analyses.

OSTI ID:
21027493
Journal Information:
Physical Review. D, Particles Fields, Vol. 76, Issue 3; Other Information: DOI: 10.1103/PhysRevD.76.033006; (c) 2007 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2821
Country of Publication:
United States
Language:
English