Neutrino spectroscopy can probe the dark matter content in the sun

Science

Volumn 330, Issue 6003, 2010, Pages 462-

  Lopes, Ilídio ^a,b   Silk, Joseph ^c,d  

^a INSTITUTO SUPERIOR TÉCNICO   (Portugal)

^b UNIVERSITY OF ÉVORA   (Portugal)

^c UNIVERSITY OF OXFORD   (United Kingdom)

^d INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

Author keywords

[No Author keywords available]

Indexed keywords

GRAVIMETRY; SOLAR ACTIVITY; SOLAR RADIATION; SPECTROSCOPY;

MOLECULAR PROBE; NEUTRINO; PARTICULATE MATTER; PRIORITY JOURNAL; SHORT SURVEY; SPECTROSCOPY; SUN; TEMPERATURE;

EID: 77958157237     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1196564     Document Type: Short Survey

References (16)

1. G. Jungman et al., Phys. Rep. 267, 195 (1996).
2. Y. Giraud-Héraud, J. Kaplan, F. Martin, C. Tao, S. Turck-Chièze, Sol. Phys. 128, 21 (1990).
3. D. Dearborn, K. Griest, G. Raffelt, Astrophys. J. 368, 626 (1991).
4. J. Kaplan, F. Martin de Volnay, C. Tao, S. Turck-Chièze, Astrophys. J. 378, 315 (1991).
5. I. P. Lopes, J. Silk, Phys. Rev. Lett. 88, 151303 (2002).
6. G. Bertone, D. Hooper, J. Silk, Phys. Rep. 405, 279 (2005).
7. S. Turck-Chièze et al., Phys. Rev. Lett. 93, 211102 (2004).
8. J. N. Bahcall, A. M. Serenelli, S. Basu, Astrophys. J. 621, L85 (2005).
9. J. A. Guzik, K. Mussack, Astrophys. J. 713, 1108 (2010).
10. M. Taoso, F. Iocco, G. Meynet, G. Bertone, P. Eggenberger, http://arxiv.org/abs/1005.5711 (2010).
11. S. Turck-Chièze et al., Astrophys. J. 604 (Issue 1), 455 (2004).
12. R. A. García et al., Science 316, 1591 (2007); published online 3 May 2007 (10.1126/science.1140598).
13. B. Aharmim et al., Phys. Rev. Lett. 101, 111301 (2008).
14. C. Arpesella et al., Phys. Rev. Lett. 101, 091302 (2008).
15. S. Turck-Chièze, A. Palacios, J. P. Marques, P. A. P. Nghiem, Astrophys. J. 715, 1539 (2010).
16. While preparing this work, we benefited from the advice of J. Guzik, S. West, and J. Dias de Deus. I.L. acknowledges the financial support of Fundação para a Ciência e a Tecnologia and Fundação Calouste Gulbenkian.