Improved limits on strongly interacting massive particles with NaI(T1) scintillators Beijing-Paris-Rome-Saclay (BPRS) Collaboration

Astroparticle Physics

Volumn 4, Issue 3, 1996, Pages 195-198

  Bacci, C ^a   Belli, P ^a   Bernabei, R ^b   Dai, C J ^c   Di Nicolantonio, W ^d   Ding, L K ^c   Gaillard Lecanu, E ^e   Gerbier, G ^e   Giraud Heraud, Y ^f   Kuang, H H ^c   Incicchitti, A ^g   Landoni, V ^b   Mallet, J ^e   Mosca, L ^e   Prosperi, D ^g   Tao, C ^f  

^a ROMA TRE UNIVERSITY   (Italy)

^b UNIVERSITY OF ROME TOR VERGATA   (Italy)

^c INSTITUTE OF GEOLOGY AND GEOPHYSICS   (China)

^d LABORATORI NAZIONALI DEL GRAN SASSO   (Italy)

^e CEA SACLAY   (France)

^f PSL Research University   (France)

^g INFN SEZIONE DI ROMA   (Italy)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 16144366893     PISSN: 09276505     EISSN: None     Source Type: Journal    
DOI: 10.1016/0927-6505(95)00032-1     Document Type: Article

References (25)

1. [1] D.N. Schramm, Nucl. Phys. B (Proc. Supp.) 28 A (1992) 243 and references quoted therein; P.P. Smith and J.D. Lewin, Phys. Rep. 187 (1990) 203; R. Bernabei, C. Tao eds, The Dark side of the Universe (World Scientific, Singapore, 1994); L. Mosca, in: Particle Astrophysics, Atomic Physics and Gravitation, (Ed. Frontières, Paris, 1994); R. Bernabei, ROM2F/94/33 to appear in Proc. of "The Standard Model and Beyond, Jaca 1994.
2. [1] D.N. Schramm, Nucl. Phys. B (Proc. Supp.) 28 A (1992) 243 and references quoted therein; P.P. Smith and J.D. Lewin, Phys. Rep. 187 (1990) 203; R. Bernabei, C. Tao eds, The Dark side of the Universe (World Scientific, Singapore, 1994); L. Mosca, in: Particle Astrophysics, Atomic Physics and Gravitation, (Ed. Frontières, Paris, 1994); R. Bernabei, ROM2F/94/33 to appear in Proc. of "The Standard Model and Beyond, Jaca 1994.
3. [1] D.N. Schramm, Nucl. Phys. B (Proc. Supp.) 28 A (1992) 243 and references quoted therein; P.P. Smith and J.D. Lewin, Phys. Rep. 187 (1990) 203; R. Bernabei, C. Tao eds, The Dark side of the Universe (World Scientific, Singapore, 1994); L. Mosca, in: Particle Astrophysics, Atomic Physics and Gravitation, (Ed. Frontières, Paris, 1994); R. Bernabei, ROM2F/94/33 to appear in Proc. of "The Standard Model and Beyond, Jaca 1994.
4. [1] D.N. Schramm, Nucl. Phys. B (Proc. Supp.) 28 A (1992) 243 and references quoted therein; P.P. Smith and J.D. Lewin, Phys. Rep. 187 (1990) 203; R. Bernabei, C. Tao eds, The Dark side of the Universe (World Scientific, Singapore, 1994); L. Mosca, in: Particle Astrophysics, Atomic Physics and Gravitation, (Ed. Frontières, Paris, 1994); R. Bernabei, ROM2F/94/33 to appear in Proc. of "The Standard Model and Beyond, Jaca 1994.
5. [1] D.N. Schramm, Nucl. Phys. B (Proc. Supp.) 28 A (1992) 243 and references quoted therein; P.P. Smith and J.D. Lewin, Phys. Rep. 187 (1990) 203; R. Bernabei, C. Tao eds, The Dark side of the Universe (World Scientific, Singapore, 1994); L. Mosca, in: Particle Astrophysics, Atomic Physics and Gravitation, (Ed. Frontières, Paris, 1994); R. Bernabei, ROM2F/94/33 to appear in Proc. of "The Standard Model and Beyond, Jaca 1994.
6. [2] G Gelmini, Nucl. Phys. B (Proc. Supp.) 28 A (1992) 254; A. Bottino et al., Phys Lett. B 265 (1991) 57; Nucl. Phys. (Proc. Supp.) 28 A (1992) 314.
7. [2] G Gelmini, Nucl. Phys. B (Proc. Supp.) 28 A (1992) 254; A. Bottino et al., Phys Lett. B 265 (1991) 57; Nucl. Phys. (Proc. Supp.) 28 A (1992) 314.
8. [2] G Gelmini, Nucl. Phys. B (Proc. Supp.) 28 A (1992) 254; A. Bottino et al., Phys Lett. B 265 (1991) 57; Nucl. Phys. (Proc. Supp.) 28 A (1992) 314.
9. [3] M.W. Goodman and E. Witten, Phys. Rev. D 31 (1985) 3059.
10. [4] S. Dimopoulus et al., Phys. Rev. D 41 (1990) 2388; A. De Rujula, S. Glashow and U. Sarid, Report No. HUTP-89/A001, (1989); P.F. Smith, Contemp. Phys. 29 (1988) 159; D. Nitz et al., in: New Frontiers in Particles Physics (World Scientific, Singapore, 1986) 1143; H. Goldberg and L.J. Hall, Phys. Lett. B 174 (1986) 151.
11. [4] S. Dimopoulus et al., Phys. Rev. D 41 (1990) 2388; A. De Rujula, S. Glashow and U. Sarid, Report No. HUTP-89/A001, (1989); P.F. Smith, Contemp. Phys. 29 (1988) 159; D. Nitz et al., in: New Frontiers in Particles Physics (World Scientific, Singapore, 1986) 1143; H. Goldberg and L.J. Hall, Phys. Lett. B 174 (1986) 151.
12. [4] S. Dimopoulus et al., Phys. Rev. D 41 (1990) 2388; A. De Rujula, S. Glashow and U. Sarid, Report No. HUTP-89/A001, (1989); P.F. Smith, Contemp. Phys. 29 (1988) 159; D. Nitz et al., in: New Frontiers in Particles Physics (World Scientific, Singapore, 1986) 1143; H. Goldberg and L.J. Hall, Phys. Lett. B 174 (1986) 151.
13. [4] S. Dimopoulus et al., Phys. Rev. D 41 (1990) 2388; A. De Rujula, S. Glashow and U. Sarid, Report No. HUTP-89/A001, (1989); P.F. Smith, Contemp. Phys. 29 (1988) 159; D. Nitz et al., in: New Frontiers in Particles Physics (World Scientific, Singapore, 1986) 1143; H. Goldberg and L.J. Hall, Phys. Lett. B 174 (1986) 151.
14. [4] S. Dimopoulus et al., Phys. Rev. D 41 (1990) 2388; A. De Rujula, S. Glashow and U. Sarid, Report No. HUTP-89/A001, (1989); P.F. Smith, Contemp. Phys. 29 (1988) 159; D. Nitz et al., in: New Frontiers in Particles Physics (World Scientific, Singapore, 1986) 1143; H. Goldberg and L.J. Hall, Phys. Lett. B 174 (1986) 151.
15. [5] G.D. Starkman et al., Phys. Rev. D 41 (1990) 3594.
16. [6] D.O. Caldwell, Nucl. Phys. B (Proc. Supp.) 28 A (1992) 273.
17. [7] C. Bacci et al., Astrop. Phys. 2 (1994) 13; R. Bernabei et al., ROM2F/94/56 to appear in Nucl Phys. B (Proc. Supp).
18. [7] C. Bacci et al., Astrop. Phys. 2 (1994) 13; R. Bernabei et al., ROM2F/94/56 to appear in Nucl Phys. B (Proc. Supp).
19. [8] K. Hikasa et al., Phys. Rev. D 45 (1992) Ill.40.
20. [9] P. Belli et al., Il Nuovo Cim. 101A (1989) 959; E. Gaillard-Lecanu, PhD thesis, Paris Sud, 1994.
21. [9] P. Belli et al., Il Nuovo Cim. 101A (1989) 959; E. Gaillard-Lecanu, PhD thesis, Paris Sud, 1994.
22. [10] H. Bilokon, private communication.
23. [11] J.I. Collar and F.T. Avignone III, Phys. Rev. D 47 (1993) 5238.
24. [12] A. Bottino et al., Phys. Lett. B 295 (1992) 330.
25. [13] J. Engel, Phys. Lett. B 264 (1991) 114.