Pregled bibliografske jedinice broj: 36627
Stringent constraint on the scalar-neutrino coupling constant from quintessential cosmology
Stringent constraint on the scalar-neutrino coupling constant from quintessential cosmology // Modern physics letters A, 14 (1999), 32; 2245-2251 (međunarodna recenzija, članak, znanstveni)
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Naslov
Stringent constraint on the scalar-neutrino coupling constant from quintessential cosmology
Autori
Horvat, Raul
Izvornik
Modern physics letters A (0217-7323) 14
(1999), 32;
2245-2251
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
quantum-field theories; equivalence principle; finite-temperature; perturbation-series; solar; relativity; gravity
Sažetak
An extremely light (m_phi 10^-33 eV), slowly-varying scalar field phi (quintessence) with a potential energy density as large as 60% of the critical density has been proposed as the origin of the accelerated expansion of the Universe at present. The interaction of this smoothly distributed component with another predominately smooth component, the cosmic neutrino background, is studied. The slow-roll approximation for generic phi potentials may then be used to obtain a limit on the scalar-neutrino coupling constant, found to be many orders of magnitude more stringent than the limits set by observations of neutrinos from SN 1987A. In addition, if quintessential theory allows for a violation of the equivalence principle in the sector of neutrinos, the current solar neutrino data can probe such a violation at the 10^-10 level.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus