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Volumn 71, Issue 6, 2005, Pages 1-14

Exploiting the neutronization burst of a galactic supernova

Author keywords

[No Author keywords available]

Indexed keywords

ACCURACY; ARTICLE; COSMOS; ELECTRON CAPTURE DETECTION; LUMINESCENCE; MATHEMATICAL ANALYSIS; MATHEMATICAL COMPUTING; MATHEMATICAL MODEL; MOLECULAR WEIGHT; NEUTRON ACTIVATION ANALYSIS; OPTICS; SIMULATION; STRUCTURE ANALYSIS;

EID: 18444367664     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.71.063003     Document Type: Article
Times cited : (156)

References (70)
  • 7
    • 0001323343 scopus 로고    scopus 로고
    • C. Lunardini and A. Y. Smirnov, Nucl. Phys. B616, 307 (2001); K. Takahashi and K. Sato, Phys. Rev. D 66, 033006 (2002); A. S. Dighe, M. T. Keil, and G. G. Raffelt, J. Cosmol. Astropart. Phys. 06 (2003) 006; A. S. Dighe, M. Kachelrieß, G. G. Raffelt, and R. Tomàs, J. Cosmol. Astropart. Phys. 01 (2004) 004.
    • (2001) Nucl. Phys. , vol.B616 , pp. 307
    • Lunardini, C.1    Smirnov, A.Y.2
  • 8
    • 0036695405 scopus 로고    scopus 로고
    • C. Lunardini and A. Y. Smirnov, Nucl. Phys. B616, 307 (2001); K. Takahashi and K. Sato, Phys. Rev. D 66, 033006 (2002); A. S. Dighe, M. T. Keil, and G. G. Raffelt, J. Cosmol. Astropart. Phys. 06 (2003) 006; A. S. Dighe, M. Kachelrieß, G. G. Raffelt, and R. Tomàs, J. Cosmol. Astropart. Phys. 01 (2004) 004.
    • (2002) Phys. Rev. D , vol.66 , pp. 033006
    • Takahashi, K.1    Sato, K.2
  • 9
    • 0001323343 scopus 로고    scopus 로고
    • C. Lunardini and A. Y. Smirnov, Nucl. Phys. B616, 307 (2001); K. Takahashi and K. Sato, Phys. Rev. D 66, 033006 (2002); A. S. Dighe, M. T. Keil, and G. G. Raffelt, J. Cosmol. Astropart. Phys. 06 (2003) 006; A. S. Dighe, M. Kachelrieß, G. G. Raffelt, and R. Tomàs, J. Cosmol. Astropart. Phys. 01 (2004) 004.
    • (2003) J. Cosmol. Astropart. Phys. , vol.6 , pp. 006
    • Dighe, A.S.1    Keil, M.T.2    Raffelt, G.G.3
  • 10
    • 0001323343 scopus 로고    scopus 로고
    • C. Lunardini and A. Y. Smirnov, Nucl. Phys. B616, 307 (2001); K. Takahashi and K. Sato, Phys. Rev. D 66, 033006 (2002); A. S. Dighe, M. T. Keil, and G. G. Raffelt, J. Cosmol. Astropart. Phys. 06 (2003) 006; A. S. Dighe, M. Kachelrieß, G. G. Raffelt, and R. Tomàs, J. Cosmol. Astropart. Phys. 01 (2004) 004.
    • (2004) J. Cosmol. Astropart. Phys. , vol.1 , pp. 004
    • Dighe, A.S.1    Kachelrieß, M.2    Raffelt, G.G.3    Tomàs, R.4
  • 11
    • 4344623309 scopus 로고    scopus 로고
    • R. C. Schirato and G. M. Fuller, astro-ph/0205390
    • R. C. Schirato and G. M. Fuller, astro-ph/0205390; G. L. Fogli, E. Lisi, D. Montanino, and A. Mirizzi, Phys. Rev. D 68, 033005 (2003).
    • (2003) Phys. Rev. D , vol.68 , pp. 033005
    • Fogli, G.L.1    Lisi, E.2    Montanino, D.3    Mirizzi, A.4
  • 14
    • 0141546601 scopus 로고
    • Neutrinos from Supernovae
    • edited by A. G. Petschek (Springer, New York)
    • For a review, see A. Burrows, Neutrinos from Supernovae, in Supernovae, edited by A. G. Petschek (Springer, New York, 1990), p. 143.
    • (1990) Supernovae , pp. 143
    • Burrows, A.1
  • 16
    • 4244002228 scopus 로고
    • S. W. Bruenn, Phys. Rev. Lett. 59, 938 (1987); R. Mayle, J. R. Wilson, and D. N. Schramm, Astrophys. J. 318, 288 (1987); E. S. Myra and A. Burrows, Astrophys. J. 364, 222 (1990); M. Rampp and H.-T. Janka, Astrophys. J. 539, L33 (2000); M. Liebendörfer, A. Mezzacappa, F. K. Thielemann, O. E. B. Messer, W. R. Hix, and S. W. Bruenn, Phys. Rev. D 63, 103004 (2001); M. Liebendörfer, O. E. B. Messer, A. Mezzacappa, S. W. Bruenn, C. Y. Cardall, and F. K. Thielemann, Astrophys. J. Suppl. Ser. 150, 263 (2000).
    • (1987) Phys. Rev. Lett. , vol.59 , pp. 938
    • Bruenn, S.W.1
  • 17
    • 4244002228 scopus 로고
    • S. W. Bruenn, Phys. Rev. Lett. 59, 938 (1987); R. Mayle, J. R. Wilson, and D. N. Schramm, Astrophys. J. 318, 288 (1987); E. S. Myra and A. Burrows, Astrophys. J. 364, 222 (1990); M. Rampp and H.-T. Janka, Astrophys. J. 539, L33 (2000); M. Liebendörfer, A. Mezzacappa, F. K. Thielemann, O. E. B. Messer, W. R. Hix, and S. W. Bruenn, Phys. Rev. D 63, 103004 (2001); M. Liebendörfer, O. E. B. Messer, A. Mezzacappa, S. W. Bruenn, C. Y. Cardall, and F. K. Thielemann, Astrophys. J. Suppl. Ser. 150, 263 (2000).
    • (1987) Astrophys. J. , vol.318 , pp. 288
    • Mayle, R.1    Wilson, J.R.2    Schramm, D.N.3
  • 18
    • 0001767879 scopus 로고
    • S. W. Bruenn, Phys. Rev. Lett. 59, 938 (1987); R. Mayle, J. R. Wilson, and D. N. Schramm, Astrophys. J. 318, 288 (1987); E. S. Myra and A. Burrows, Astrophys. J. 364, 222 (1990); M. Rampp and H.-T. Janka, Astrophys. J. 539, L33 (2000); M. Liebendörfer, A. Mezzacappa, F. K. Thielemann, O. E. B. Messer, W. R. Hix, and S. W. Bruenn, Phys. Rev. D 63, 103004 (2001); M. Liebendörfer, O. E. B. Messer, A. Mezzacappa, S. W. Bruenn, C. Y. Cardall, and F. K. Thielemann, Astrophys. J. Suppl. Ser. 150, 263 (2000).
    • (1990) Astrophys. J. , vol.364 , pp. 222
    • Myra, E.S.1    Burrows, A.2
  • 19
    • 0034632321 scopus 로고    scopus 로고
    • S. W. Bruenn, Phys. Rev. Lett. 59, 938 (1987); R. Mayle, J. R. Wilson, and D. N. Schramm, Astrophys. J. 318, 288 (1987); E. S. Myra and A. Burrows, Astrophys. J. 364, 222 (1990); M. Rampp and H.-T. Janka, Astrophys. J. 539, L33 (2000); M. Liebendörfer, A. Mezzacappa, F. K. Thielemann, O. E. B. Messer, W. R. Hix, and S. W. Bruenn, Phys. Rev. D 63, 103004 (2001); M. Liebendörfer, O. E. B. Messer, A. Mezzacappa, S. W. Bruenn, C. Y. Cardall, and F. K. Thielemann, Astrophys. J. Suppl. Ser. 150, 263 (2000).
    • (2000) Astrophys. J. , vol.539
    • Rampp, M.1    Janka, H.-T.2
  • 20
    • 0034899489 scopus 로고    scopus 로고
    • S. W. Bruenn, Phys. Rev. Lett. 59, 938 (1987); R. Mayle, J. R. Wilson, and D. N. Schramm, Astrophys. J. 318, 288 (1987); E. S. Myra and A. Burrows, Astrophys. J. 364, 222 (1990); M. Rampp and H.-T. Janka, Astrophys. J. 539, L33 (2000); M. Liebendörfer, A. Mezzacappa, F. K. Thielemann, O. E. B. Messer, W. R. Hix, and S. W. Bruenn, Phys. Rev. D 63, 103004 (2001); M. Liebendörfer, O. E. B. Messer, A. Mezzacappa, S. W. Bruenn, C. Y. Cardall, and F. K. Thielemann, Astrophys. J. Suppl. Ser. 150, 263 (2000).
    • (2001) Phys. Rev. D , vol.63 , pp. 103004
    • Liebendörfer, M.1    Mezzacappa, A.2    Thielemann, F.K.3    Messer, O.E.B.4    Hix, W.R.5    Bruenn, S.W.6
  • 21
    • 1642330135 scopus 로고    scopus 로고
    • S. W. Bruenn, Phys. Rev. Lett. 59, 938 (1987); R. Mayle, J. R. Wilson, and D. N. Schramm, Astrophys. J. 318, 288 (1987); E. S. Myra and A. Burrows, Astrophys. J. 364, 222 (1990); M. Rampp and H.-T. Janka, Astrophys. J. 539, L33 (2000); M. Liebendörfer, A. Mezzacappa, F. K. Thielemann, O. E. B. Messer, W. R. Hix, and S. W. Bruenn, Phys. Rev. D 63, 103004 (2001); M. Liebendörfer, O. E. B. Messer, A. Mezzacappa, S. W. Bruenn, C. Y. Cardall, and F. K. Thielemann, Astrophys. J. Suppl. Ser. 150, 263 (2000).
    • (2000) Astrophys. J. Suppl. Ser. , vol.150 , pp. 263
    • Liebendörfer, M.1    Messer, O.E.B.2    Mezzacappa, A.3    Bruenn, S.W.4    Cardall, C.Y.5    Thielemann, F.K.6
  • 26
    • 84927705088 scopus 로고    scopus 로고
    • note
    • In the supernova simulations discussed here muon and tau neutrinos and antineutrinos are treated equally because their interaction with supernova matter is very similar. This has several reasons. On the one hand muons are not present initially or at subnuclear densities in the supernova core and taus cannot be produced at supernova conditions. On the other hand neutrino oscillations are suppressed at the high densities of the core.
  • 28
    • 84927705087 scopus 로고    scopus 로고
    • M. Liebendörfer, M. Rampp, H.-T. Janka, and A. Mezzacappa, astro-ph/0310662
    • M. Liebendörfer, M. Rampp, H.-T. Janka, and A. Mezzacappa, astro-ph/0310662.
  • 29
    • 0001971387 scopus 로고
    • Model n13
    • K. Nomoto and M. Hashimoto, Phys. Rep. 163, 13 (1988) (Model n13); S. E. Woosley and T. A. Weaver, Astrophys. J. Suppl. Ser. 101, 181 (1995) (Model s15s7b2); S. E. Woosley, A. Heger, and T. A. Weaver, Rev. Mod. Phys. 74, 1015 (2002) (Models s11.2, s20, s15a28, s25a28); M. Limongi, O. Straniero, and A. Chieffi, Astrophys. J. Suppl. Ser. 129, 625 (2000) (Models l15, l25).
    • (1988) Phys. Rep. , vol.163 , pp. 13
    • Nomoto, K.1    Hashimoto, M.2
  • 30
    • 4244154905 scopus 로고
    • Model s15s7b2
    • K. Nomoto and M. Hashimoto, Phys. Rep. 163, 13 (1988) (Model n13); S. E. Woosley and T. A. Weaver, Astrophys. J. Suppl. Ser. 101, 181 (1995) (Model s15s7b2); S. E. Woosley, A. Heger, and T. A. Weaver, Rev. Mod. Phys. 74, 1015 (2002) (Models s11.2, s20, s15a28, s25a28); M. Limongi, O. Straniero, and A. Chieffi, Astrophys. J. Suppl. Ser. 129, 625 (2000) (Models l15, l25).
    • (1995) Astrophys. J. Suppl. Ser. , vol.101 , pp. 181
    • Woosley, S.E.1    Weaver, T.A.2
  • 31
    • 0036822785 scopus 로고    scopus 로고
    • Models s11.2, s20, s15a28, s25a28
    • K. Nomoto and M. Hashimoto, Phys. Rep. 163, 13 (1988) (Model n13); S. E. Woosley and T. A. Weaver, Astrophys. J. Suppl. Ser. 101, 181 (1995) (Model s15s7b2); S. E. Woosley, A. Heger, and T. A. Weaver, Rev. Mod. Phys. 74, 1015 (2002) (Models s11.2, s20, s15a28, s25a28); M. Limongi, O. Straniero, and A. Chieffi, Astrophys. J. Suppl. Ser. 129, 625 (2000) (Models l15, l25).
    • (2002) Rev. Mod. Phys. , vol.74 , pp. 1015
    • Woosley, S.E.1    Heger, A.2    Weaver, T.A.3
  • 32
    • 0041951792 scopus 로고    scopus 로고
    • Models l15, l25
    • K. Nomoto and M. Hashimoto, Phys. Rep. 163, 13 (1988) (Model n13); S. E. Woosley and T. A. Weaver, Astrophys. J. Suppl. Ser. 101, 181 (1995) (Model s15s7b2); S. E. Woosley, A. Heger, and T. A. Weaver, Rev. Mod. Phys. 74, 1015 (2002) (Models s11.2, s20, s15a28, s25a28); M. Limongi, O. Straniero, and A. Chieffi, Astrophys. J. Suppl. Ser. 129, 625 (2000) (Models l15, l25).
    • (2000) Astrophys. J. Suppl. Ser. , vol.129 , pp. 625
    • Limongi, M.1    Straniero, O.2    Chieffi, A.3
  • 35
    • 18444410075 scopus 로고    scopus 로고
    • Ph.D. thesis, University of Tennessee
    • O. E. B. Messer, Ph.D. thesis, University of Tennessee, 2000; Bull. Am. Astron. Soc. 33, 1411 (2001).
    • (2000)
    • Messer, O.E.B.1
  • 36
    • 84927763896 scopus 로고    scopus 로고
    • O. E. B. Messer, Ph.D. thesis, University of Tennessee, 2000; Bull. Am. Astron. Soc. 33, 1411 (2001).
    • (2001) Bull. Am. Astron. Soc. , vol.33 , pp. 1411
  • 41
    • 44949275249 scopus 로고
    • J. M. Lattimer, C. J. Pethick, D. G. Ravenhall, and D. Q. Lamb, Nucl. Phys. A432, 646 (1985); J. M. Lattimer and F. D. Swesty, Nucl. Phys. A535, 331 (1991).
    • (1991) Nucl. Phys. , vol.A535 , pp. 331
    • Lattimer, J.M.1    Swesty, F.D.2
  • 43
    • 18444407586 scopus 로고    scopus 로고
    • Diploma thesis, Technische Universität München (TUM)
    • A. Marek, Diploma thesis, Technische Universität München (TUM), 2003.
    • (2003)
    • Marek, A.1
  • 46
    • 0032271676 scopus 로고    scopus 로고
    • nucl-th/980609
    • H. Shen, H. Toki, K. Oyamatsu, and K. Sumiyoshi, Nucl. Phys. A637, 435 (1998); Prog. Theor. Phys. 100, 1013 (1998); nucl-th/980609.
    • (1998) Prog. Theor. Phys. , vol.100 , pp. 1013
  • 47
    • 0001775805 scopus 로고
    • W. Hillebrandt, R. G. Wolff, and K. Nomoto, Astron. Astrophys. 133, 175 (1984); W. Hillebrandt and R. G. Wolff, in Nucleosynthesis: Challenges and New Developments, edited by W. D. Arnett and J. W. Truran (University of Chicago, Chicago, 1985), p. 131.
    • (1984) Astron. Astrophys. , vol.133 , pp. 175
    • Hillebrandt, W.1    Wolff, R.G.2    Nomoto, K.3
  • 48
    • 0001784237 scopus 로고
    • edited by W. D. Arnett and J.W. Truran (University of Chicago, Chicago)
    • W. Hillebrandt, R. G. Wolff, and K. Nomoto, Astron. Astrophys. 133, 175 (1984); W. Hillebrandt and R. G. Wolff, in Nucleosynthesis: Challenges and New Developments, edited by W. D. Arnett and J. W. Truran (University of Chicago, Chicago, 1985), p. 131.
    • (1985) Nucleosynthesis: Challenges and New Developments , pp. 131
    • Hillebrandt, W.1    Wolff, R.G.2
  • 50
    • 84927705086 scopus 로고    scopus 로고
    • A. Heger, S. E. Woosley, and H. C. Spruit, astro-ph/0409422
    • A. Heger, S. E. Woosley, and H. C. Spruit, astro-ph/0409422.
  • 56
    • 3343021670 scopus 로고
    • H. -T. Janka and R. Mönchmeyer, Astron. Astrophys. 209, L5 (1989); Astron. Astrophys. 226, 69 (1989).
    • (1989) Astron. Astrophys. , vol.226 , pp. 69
  • 57
    • 84927705085 scopus 로고    scopus 로고
    • note
    • Neutrino decays and magnetic moments introduce transitions ve → v̄e and are therefore more easily detectable. For a discussion of these possibilities, see Refs. [42-44].
  • 60
  • 61
    • 84927705084 scopus 로고    scopus 로고
    • note
    • The values of the neutrino mass differences used in the numerical analysis are Δmatm2 = 2.6 × 10-3 eV2 and Δm2 = 8.3 × 10 -5 eV2.
  • 62
    • 84927705083 scopus 로고    scopus 로고
    • http://www.sno.phy.queensu.ca
  • 65
    • 84927705082 scopus 로고    scopus 로고
    • private communication
    • P. Mazzali (private communication).
    • Mazzali, P.1
  • 66
    • 84927705081 scopus 로고    scopus 로고
    • Y. Itow et al., hep-ex/0106019
    • Y. Itow et al., hep-ex/0106019.
  • 67
    • 18444377691 scopus 로고    scopus 로고
    • Physics Potential and Feasibility of UNO
    • The UNO whitepaper, Physics Potential and Feasibility of UNO, available at http://ale.physics.sunysb.edu/uno.
    • The UNO Whitepaper
  • 69
    • 0036630716 scopus 로고    scopus 로고
    • R. Tomàs, D. Semikoz, G. G. Raffelt, M. Kachelrieß, and A. S. Dighe, Phys. Rev. D 68, 093013 (2003); The neutralcurrent events on oxygen have been simulated following E. Kolbe, K. Langanke, and P. Vogel, Phys. Rev. D 66, 013007 (2002).
    • (2002) Phys. Rev. D , vol.66 , pp. 013007
    • Kolbe, E.1    Langanke, K.2    Vogel, P.3


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