https://doi.org/10.1140/epjc/s10052-008-0530-9
Regular Article - Experimental Physics
Search for solar axions emitted in the M1-transition of 7Li* with Borexino CTF
1
Dipartimento di Fisica Università and INFN Milano, Via Celoria 16, 20133, Milano, Italy
2
Department of Chemical Engineering, A-217, Engineering Quadrangle, Princeton, NJ, 08544-0708, USA
3
Department of Physics, Princeton University, Jadwin Hall, Washington Rd, Princeton, NJ, 08544-0708, USA
4
Astroparticule et Cosmologie APC, 10 rue Alice Domon et Leonie Duquet, 75205, Paris cedex 13, France
5
St. Petersburg Nuclear Physics Institute, 188300, Gatchina, Russia
6
RRC Kurchatov Institute, Kurchatov Sq.1, 123182, Moscow, Russia
7
Joint Institute for Nuclear Research, Joliot Curie 6, 141980, Dubna, Moscow region, Russia
8
INFN Laboratori Nazionali del Gran Sasso, SS 17 bis Km 18+910, 67010, Assergi (AQ), Italy
9
Technische Universität München, James Franck Strasse, E15, 85747, Garching, Germany
10
Physics Department, Virginia Polytechnic Institute and State University, Roberson Hall, Blacksburg, VA, 24061-0435, USA
11
Kiev Institute for Nuclear Research, 47 Prospekt Nauki, 06380, Kiev, Ukraine
12
Dipartimento di Fisica Università and I.N.F.N. Genova, Via Dodecaneso 33, 16146, Genova, Italy
13
Dipartimento di Chimica Università di Perugia, Via Elce di Sotto 8, 06123, Perugia, Italy
14
M. Smoluchowski Institute of Physics, Jagellonian University, ul. Reymonta 4, 30059, Krakow, Poland
15
Max-Planck-Institut für Kernphysik, Postfach 103 980, 69029, Heidelberg, Germany
* e-mail: derbin@pnpi.spb.ru
Received:
20
August
2007
Published online:
29
January
2008
Results of background measurements with a prototype of the Borexino detector were used to search for 478 keV solar axions emitted in the M1-transitions of 7Li*. The Compton conversion of axion to a photon A+e→e+γ, axioelectric effect A+e+Z→e+Z, decay of axion in two photons A→2γ and Primakoff conversion on nuclei A+Z→γ+Z are considered. The upper limit on constants of interaction of axion with electrons, photons and nucleons – gAegAN≤(1.0–2.4)×10-10 at mA≤450 keV and gAγgAN≤5×10-9 GeV-1 at mA≤10 keV are obtained (90%c.l.). For heavy axions with mass at 100<mA<400 keV the limits gAe<(0.7–2.0)×10-8 and gAγ<10-9–10-8 are obtained in assumption that gAN depends on mA as for KSVZ axion model. These limits are stronger than obtained in previous laboratory-based experiments using nuclear reactor and artificial radioactive sources.
© Springer-Verlag , 2008