Supernova bounds on supersymmetric R-parity violating interactions

Nuclear Physics B

Volumn 482, Issue 1-2, 1996, Pages 481-494

  Nunokawa, H ^a   Rossi, A ^a   Valle, J W F ^a  

^a UNIVERSITY OF VALENCIA   (Spain)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0030599639     PISSN: 05503213     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0550-3213(96)00541-X     Document Type: Article

References (52)

1. [1] L. Wolfenstein, Phys. Rev. D 17 (1978) 2369.
2. [2] J.W.F. Valle, Phys. Lett. B 199 (1987) 432.
3. [3] E. Roulet, Phys. Rev. D 44 (1991) R2935.
4. [4] M.M. Guzzo, A. Masiero and S.T. Petcov, Phys. Lett. B 260 (1991) 154.
5. [5] S.P. Mikheyev and A.Yu. Smirnov, Sov. J. Nucl. Phys. 42 (1985) 913.
6. [6] A.Yu. Smirnov, in Proc. of the 4th Int. Symp. on Neutrino Telescopes, Venice, Italy, ed. M. Baldo Ceolin (University of Padova, 1992) p. 63.
7. [7] H. Nunokawa, Y.-Z. Qian, A. Rossi and J.W.F. Valle, Phys. Rev. D 54 (1996) 4356.
8. [8] V. Barger, R.J.N. Phillips and K. Whisnant, Phys. Rev. D 44 (1991) 1629; S. Degl' Innocenti and B. Ricci, Mod. Phys. Lett. A 8 (1993) 471.
9. [8] V. Barger, R.J.N. Phillips and K. Whisnant, Phys. Rev. D 44 (1991) 1629; S. Degl' Innocenti and B. Ricci, Mod. Phys. Lett. A 8 (1993) 471.
10. [9] For a recent review see J.W.F. Valle, in Physics Beyond the Standard Model, lectures given at the VIII Jorge Andre Swieca Summer School (Rio de Janeiro, February 1995) and at V Taller Latinoamericano de Fenomenologia de las Interacciones Fundamentales (Puebla, Mexico, October 1995); hep-ph/9603307.
11. [10] S. Weinberg, Phys. Rev. D 26 (1982) 287.
12. [11] C. Aulak and N.R. Mohapatra, Phys. Lett. B 119 (1983) 136; F. Zwirner, Phys. Lett. B 132 (1983) 103; L.J. Hall and M. Suzuki, Nucl. Phys. B 231 (1984) 419; J. Ellis et al., Phys. Lett. B 150 (1985) 142; G.G. Ross and J.W.F. Valle, Phys. Lett. B 151 (1985) 375; R. Barbieri and A. Masiero, Phys. Lett. B 267 (1986) 679.
13. [11] C. Aulak and N.R. Mohapatra, Phys. Lett. B 119 (1983) 136; F. Zwirner, Phys. Lett. B 132 (1983) 103; L.J. Hall and M. Suzuki, Nucl. Phys. B 231 (1984) 419; J. Ellis et al., Phys. Lett. B 150 (1985) 142; G.G. Ross and J.W.F. Valle, Phys. Lett. B 151 (1985) 375; R. Barbieri and A. Masiero, Phys. Lett. B 267 (1986) 679.
14. [11] C. Aulak and N.R. Mohapatra, Phys. Lett. B 119 (1983) 136; F. Zwirner, Phys. Lett. B 132 (1983) 103; L.J. Hall and M. Suzuki, Nucl. Phys. B 231 (1984) 419; J. Ellis et al., Phys. Lett. B 150 (1985) 142; G.G. Ross and J.W.F. Valle, Phys. Lett. B 151 (1985) 375; R. Barbieri and A. Masiero, Phys. Lett. B 267 (1986) 679.
15. [11] C. Aulak and N.R. Mohapatra, Phys. Lett. B 119 (1983) 136; F. Zwirner, Phys. Lett. B 132 (1983) 103; L.J. Hall and M. Suzuki, Nucl. Phys. B 231 (1984) 419; J. Ellis et al., Phys. Lett. B 150 (1985) 142; G.G. Ross and J.W.F. Valle, Phys. Lett. B 151 (1985) 375; R. Barbieri and A. Masiero, Phys. Lett. B 267 (1986) 679.
16. [11] C. Aulak and N.R. Mohapatra, Phys. Lett. B 119 (1983) 136; F. Zwirner, Phys. Lett. B 132 (1983) 103; L.J. Hall and M. Suzuki, Nucl. Phys. B 231 (1984) 419; J. Ellis et al., Phys. Lett. B 150 (1985) 142; G.G. Ross and J.W.F. Valle, Phys. Lett. B 151 (1985) 375; R. Barbieri and A. Masiero, Phys. Lett. B 267 (1986) 679.
17. [11] C. Aulak and N.R. Mohapatra, Phys. Lett. B 119 (1983) 136; F. Zwirner, Phys. Lett. B 132 (1983) 103; L.J. Hall and M. Suzuki, Nucl. Phys. B 231 (1984) 419; J. Ellis et al., Phys. Lett. B 150 (1985) 142; G.G. Ross and J.W.F. Valle, Phys. Lett. B 151 (1985) 375; R. Barbieri and A. Masiero, Phys. Lett. B 267 (1986) 679.
18. [12] Y.-Z. Qian et al., Phys. Rev. Lett. 71 (1993) 1965.
19. [13] P. Reinartz and L. Stodolsky, Z. Physik C 27 (1985) 507; L. Wolfenstein, Phys. Lett. B 194 (1987) 197.
20. [13] P. Reinartz and L. Stodolsky, Z. Physik C 27 (1985) 507; L. Wolfenstein, Phys. Lett. B 194 (1987) 197.
21. [14] A. Yu. Smirnov, D.N. Spergel and J.N. Bahcall, Phys. Rev. D 49 (1994) 1389.
22. [15] B. Jegerlehner, F. Neubig and G. Raffelt, Phys. Rev. D 54 (1996) 1194.
23. [16] See for a review, e.g., H. Haber and G. Kane, Phys. Rep. 117 (1985) 75; H.P. Nilles, Phys. Rep. 110 (1984) 1; R. Barbieri, Riv. del Nuovo Cim.-11 (1988) 1.
24. [16] See for a review, e.g., H. Haber and G. Kane, Phys. Rep. 117 (1985) 75; H.P. Nilles, Phys. Rep. 110 (1984) 1; R. Barbieri, Riv. del Nuovo Cim.-11 (1988) 1.
25. [16] See for a review, e.g., H. Haber and G. Kane, Phys. Rep. 117 (1985) 75; H.P. Nilles, Phys. Rep. 110 (1984) 1; R. Barbieri, Riv. del Nuovo Cim.-11 (1988) 1.
26. [17] V. Barger, G.F. Giudice and T. Han, Phys. Rev. D 40 (1989) 2987; C.E. Carlson, P. Roy and M. Sher, Phys. Lett. B 357 (1995) 99; D. Choudhury and P. Roy, Phys. Lett. B 378 (1996) 153.
27. [17] V. Barger, G.F. Giudice and T. Han, Phys. Rev. D 40 (1989) 2987; C.E. Carlson, P. Roy and M. Sher, Phys. Lett. B 357 (1995) 99; D. Choudhury and P. Roy, Phys. Lett. B 378 (1996) 153.
28. [17] V. Barger, G.F. Giudice and T. Han, Phys. Rev. D 40 (1989) 2987; C.E. Carlson, P. Roy and M. Sher, Phys. Lett. B 357 (1995) 99; D. Choudhury and P. Roy, Phys. Lett. B 378 (1996) 153.
29. [18] A.Yu. Smirnov and F. Vissani, Phys. Lett. B 380 (1996) 317.
30. [19] G. Bhattacharyya, preprint hep-ph/9511447, to appear in the Proc. of the HEP Conf., Brussels, 1995.
31. [20] R. Mohapatra, Phys. Rev. Lett. 75 (1995) 2276; M. Hirsch, H.V. Kapodor-Kleigrothaus and S.G. Kovalenko Phys. Lett. B 372 (1996) 181.
32. [20] R. Mohapatra, Phys. Rev. Lett. 75 (1995) 2276; M. Hirsch, H.V. Kapodor-Kleigrothaus and S.G. Kovalenko Phys. Lett. B 372 (1996) 181.
33. [21] L. Landau, Phys. Z. Sowjetunion 2 (1932) 46; C. Zener, Proc. R. Soc. London A 137 (1932) 696.
34. [21] L. Landau, Phys. Z. Sowjetunion 2 (1932) 46; C. Zener, Proc. R. Soc. London A 137 (1932) 696.
35. [22] W.C. Haxton, Phys. Rev. Lett. 57 (1986) 1271; S.J. Parke, Phys. Rev. Lett. 57 (1986) 1275; A. Dar et al., Phys. Rev. D 35 (1987) 3607.
36. [22] W.C. Haxton, Phys. Rev. Lett. 57 (1986) 1271; S.J. Parke, Phys. Rev. Lett. 57 (1986) 1275; A. Dar et al., Phys. Rev. D 35 (1987) 3607.
37. [22] W.C. Haxton, Phys. Rev. Lett. 57 (1986) 1271; S.J. Parke, Phys. Rev. Lett. 57 (1986) 1275; A. Dar et al., Phys. Rev. D 35 (1987) 3607.
38. [23] K. Hirata et al., Phys. Rev. Lett. 58 (1987) 1490.
39. [24] R. Bionta et al., Phys. Rev. Lett. 58 (1987) 1494.
40. [25] S.E. Woosley and E. Baron, Astrophys. J. 391 (1992) 228; S.E. Woosley, Astron. Astrophys. Suppl. Ser. 97 (1993) 205; S.E. Woosley and R.D. Hoffman, Astrophys. J. 395 (1992) 202; B.S. Meyer et al., Astrophys. J. 399 (1992) 656; S.E. Woosley et al., Astrophys. J. 433 (1994) 229.
41. [25] S.E. Woosley and E. Baron, Astrophys. J. 391 (1992) 228; S.E. Woosley, Astron. Astrophys. Suppl. Ser. 97 (1993) 205; S.E. Woosley and R.D. Hoffman, Astrophys. J. 395 (1992) 202; B.S. Meyer et al., Astrophys. J. 399 (1992) 656; S.E. Woosley et al., Astrophys. J. 433 (1994) 229.
42. [25] S.E. Woosley and E. Baron, Astrophys. J. 391 (1992) 228; S.E. Woosley, Astron. Astrophys. Suppl. Ser. 97 (1993) 205; S.E. Woosley and R.D. Hoffman, Astrophys. J. 395 (1992) 202; B.S. Meyer et al., Astrophys. J. 399 (1992) 656; S.E. Woosley et al., Astrophys. J. 433 (1994) 229.
43. [25] S.E. Woosley and E. Baron, Astrophys. J. 391 (1992) 228; S.E. Woosley, Astron. Astrophys. Suppl. Ser. 97 (1993) 205; S.E. Woosley and R.D. Hoffman, Astrophys. J. 395 (1992) 202; B.S. Meyer et al., Astrophys. J. 399 (1992) 656; S.E. Woosley et al., Astrophys. J. 433 (1994) 229.
44. [25] S.E. Woosley and E. Baron, Astrophys. J. 391 (1992) 228; S.E. Woosley, Astron. Astrophys. Suppl. Ser. 97 (1993) 205; S.E. Woosley and R.D. Hoffman, Astrophys. J. 395 (1992) 202; B.S. Meyer et al., Astrophys. J. 399 (1992) 656; S.E. Woosley et al., Astrophys. J. 433 (1994) 229.
45. [26] For reviews, see R. Rowan-Robinson, in Cosmological Dark Matter, ed. J.W.F. Valle and A. Perez (World Scientific, Singapore, 1994) p. 7; C.S. Frenk, in Cosmological Dark Matter, ed. J.W.F. Valle and A. Perez (World Scientific, Singapore, 1994) p. 65; J. Primack in Cosmological Dark Matter, ed. J.W.F. Valle and A. Perez (World Scientific, Singapore, 1994) p. 81.
46. [26] For reviews, see R. Rowan-Robinson, in Cosmological Dark Matter, ed. J.W.F. Valle and A. Perez (World Scientific, Singapore, 1994) p. 7; C.S. Frenk, in Cosmological Dark Matter, ed. J.W.F. Valle and A. Perez (World Scientific, Singapore, 1994) p. 65; J. Primack in Cosmological Dark Matter, ed. J.W.F. Valle and A. Perez (World Scientific, Singapore, 1994) p. 81.
47. [26] For reviews, see R. Rowan-Robinson, in Cosmological Dark Matter, ed. J.W.F. Valle and A. Perez (World Scientific, Singapore, 1994) p. 7; C.S. Frenk, in Cosmological Dark Matter, ed. J.W.F. Valle and A. Perez (World Scientific, Singapore, 1994) p. 65; J. Primack in Cosmological Dark Matter, ed. J.W.F. Valle and A. Perez (World Scientific, Singapore, 1994) p. 81.
48. [27] A.I. Belesev et al., Phys. Lett. B 350 (1995) 263.
49. [28] For a recent overview and earlier references, see A. Burrows, astro-ph/9606035.
50. [29] H.A. Bethe and J.R. Wilson, Astrophys. J. 307 (1986) 178.
51. [30] G.M. Fuller et al., Astrophys. J. 389 (1992) 517.
52. [31] E.Kh. Akhmedov, A. Lanza, S.T. Petcov and D.W. Sciama, SISSA-40-96-A-EP; TUM-HEP-239-96; hep-ph/9603443.