A next-generation liquid-scintillator detector will be able to perform high-statistics measurements of the solar neutrino flux. In LENA, solar 7Be neutrinos are expected to cause 1.7×104 electron recoil events per day in a fiducial volume of 35 kilotons. Based on this signal, a search for periodic modulations on a subpercent level can be conducted, surpassing the sensitivity of current detectors by at least a factor of 20. The range of accessible periods reaches from several minutes, corresponding to modulations induced by helioseismic g-modes, to tens of years, allowing to study long-term changes in solar fusion rates.

Search for modulations of the solar 7Be flux in the next-generation neutrino observatory LENA / M. Wurm, B. Caccianiga, D. D’Angelo, S. Davini, F. von Feilitzsch, M. Göger Neff, T. Lachenmaier, T. Lewke, P. Lombardi, L. Ludhova, Q. Meindl, E. Meroni, L. Miramonti, R. Möllenberg, L. Oberauer, W. Potzel, G. Ranucci, M. Tippmann, J. Winter. - In: PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. - ISSN 1550-7998. - 83:3(2011 Feb 24), pp. 032010.032010.1-032010.032010.11. [10.1103/PhysRevD.83.032010]

Search for modulations of the solar 7Be flux in the next-generation neutrino observatory LENA

B. Caccianiga
Secondo
;
D. D’Angelo;E. Meroni;L. Miramonti;
2011

Abstract

A next-generation liquid-scintillator detector will be able to perform high-statistics measurements of the solar neutrino flux. In LENA, solar 7Be neutrinos are expected to cause 1.7×104 electron recoil events per day in a fiducial volume of 35 kilotons. Based on this signal, a search for periodic modulations on a subpercent level can be conducted, surpassing the sensitivity of current detectors by at least a factor of 20. The range of accessible periods reaches from several minutes, corresponding to modulations induced by helioseismic g-modes, to tens of years, allowing to study long-term changes in solar fusion rates.
solar neutrino flux ; liquid-scintillator detector
Settore FIS/01 - Fisica Sperimentale
Settore FIS/04 - Fisica Nucleare e Subnucleare
Settore FIS/05 - Astronomia e Astrofisica
24-feb-2011
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2434/154680
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