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The Physics of Supernovae

Published online by Cambridge University Press:  12 April 2016

S.E. Woosley  and
Thomas A. Weaver
S.E. Woosley
Affiliation:
Board of Studies in Astronomy and Astrophysics Lick Observatory, University of California at Santa Cruz, Santa Cruz CA 95064 and Special Studies Group, Lawrence Livermore National Laboratory, Livermore CA 94550
Thomas A. Weaver
Affiliation:
Special Studies Group, Lawrence Livermore National Laboratory, University of California, Livermore CA 94550

Abstract

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Presupernova models of massive stars are presented and their explosion by “delayed neutrino transport” examined. A new form of long duration Type II supernova model is also explored based upon repeated encounter with the electron-positron pair instability in stars heavier than about 60 M⊙. Carbon deflagration in white dwarfs is discussed as the probable explanation of Type I supernovae and special attention is paid to the physical processes whereby a nuclear flame propagates through degenerate carbon.

Type
3. Supernovae
Information
International Astronomical Union Colloquium , Volume 89: Radiation Hydrodynamics in Stars and Compacts Objects , 1986 , pp. 90 - 120
Copyright
Copyright © Springer-Verlag 1986

References

Arnett, W.D. 1979, Ap. J. Lett. 230:L37.Google Scholar
Arnett, W.D. 1983, Ap. J. Lettr. 263:L55.Google Scholar
Arnett, W.D. 1985, Preprint Enrico Fermi Inst., Univ. Chicago, submitted to Ap. J. Lettr.Google Scholar
Axelrod, T.S. 1980a, Ph.D. Thesis UCSC, available as UCRL preprint 52994 from Lawrence Livermore National Laboratory.Google Scholar
Axelrod, T.S. 1980b, Type I Supernovae, ed. Wheeler, J.C.. Austin: Univ. of Texas, p. 80.Google Scholar
Barkat, Z., Rakavy, G., and Sack, N. 1967, Phys. Rev. Lettr. 19:379.Google Scholar
Barkat, Z., Reiss, Y., and Rakavy, G. 1974, Ap. J. Lettr. 193:L21.CrossRefGoogle Scholar
Baron, E., Cooperstein, J., and Kahana, S. 1985a, Phys. Rev. Lettr. 55:126.CrossRefGoogle Scholar
Baron, E., Cooperstein, J., and Kahana, S. 1985b, Nucl. Phys., A440:744.Google Scholar
Baron, E., Brown, G.E., Cooperstein, J., and Prakash, M. 1985, Preprint.Google Scholar
Berteli, G., Bressan, A.G., and Chiosi, C. 1984, Astron. and Ap. 130:279.Google Scholar
Berteli, G., Bressan, A.G., and Chiosi, C. 1985, Astron. and Ap. 150:33.Google Scholar
Bethe, H.A. 1985, private communication.Google Scholar
Bethe, H.A., and Wilson, J.R. 1985, Ap. J. 295:14.Google Scholar
Bodenheimer, P., and Woosley, S.E. 1983, Ap. J. 269:281.Google Scholar
Bowers, R.L. 1985, private communication.Google Scholar
Bowers, R.L., and Wilson, J.R. 1982, Ap. J. 263:366.Google Scholar
Branch, D. 1984a, Ann. N. Y. Acad. Sci. 422:186.Google Scholar
Branch, D. 1984b, Stellar Nucleosynthesis, eds. Chiosi, C. and Renzini, A.. D. Reidel: Dordrecht. p. 19.CrossRefGoogle Scholar
Branch, D., and Greenstein, J.L. 1971, Ap. J. 167:89.CrossRefGoogle Scholar
Branch, D., Doggett, J.B., Nomoto, K., and Thielemann, F.-K. 1985, Ap. J., 294:619.Google Scholar
Brown, G.E., Bethe, H.A., and Baym, G. 1982, Nucl. Phys. A375:481.Google Scholar
Bruenn, S.W. 1985, Ap. J. Suppl. 58:771.Google Scholar
Burrows, A. and Lattimer, J.M. 1985, Ap. J., in press.Google Scholar
Cameron, A.G.W. 1982, Essays in Nuclear Astrophysics, ed. Barnes, C., Clayton, D., and Schramm, D., Cambridge Univ. Press: Cambridge, p. 23.Google Scholar
Chevalier, R.A. 1976, Ap. J. 208:826.Google Scholar
Chevalier, R.A. 1981, Ap. J. 246:267.Google Scholar
Chiosi, C. 1981, The Most Massive Stars, ESO Workshop, ed. D’Odorico, S., Baade, D., and Kaeyer, K.. ESO: Garching. p. 27.Google Scholar
Colgate, S.A., and McKee, C. 1969, Ap. J. 157:623.Google Scholar
Conti, P.S., Leep, E.M., and Perry, D.N. 1983, Ap. J. 268:228.Google Scholar
Filippenko, A.V., and Sargent, W.L.W. 1985, Nature. 316:407.CrossRefGoogle Scholar
Firmani, C. 1982, In WR Stars: Observations, Physics, and Evolution, IAU Colloq. 99, ed. deLoore, C. and Willis, A.J., p. 499.Google Scholar
Graham, J.R., Meikle, W.P.S., Allen, D.A., Longmore, A.J., and Williams, P.M. 1985, M.N.R.A.S. In press.Google Scholar
Hartmann, D.H., Woosley, S.E., and El Eid, M. 1985, Ap. J. 297:837.Google Scholar
Hillebrandt, W. 1984, Ann. N. Y. Acad. Sci. 422:197.Google Scholar
Hillebrandt, W. 1985, To appear in Cosmogonical Processes, proceedings of A. G. W. Cameron’s 60th Birthday symposium, Boulder, Colorado.Google Scholar
Hillebrandt, W., Nomoto, K., and Wolff, R.G. 1984, Astron. Ap. 133:175.Google Scholar
Humphreys, R.M. 1984, Observational Tests of the Stellar Evolution Theory, IAU Proc. 105, ed. Maeder, A. and Renzini, A., D. Reidel: Dordrecht, p. 279.Google Scholar
Iben, I. 1985, Quart. J. Roy. Astron. Soc. 26:1.Google Scholar
Iben, I. Jr., and Renzini, A. 1983, Ann. Rev. Astron, and Ap. 21:271.Google Scholar
Iben, I. Jr. and Tutukov, A.V. 1984, Ap. J. Suppl. Ser. 54:335.Google Scholar
Iben, I. Jr. and Tutukov, A.V. 1985, Ap. J. Suppl. 58:661.Google Scholar
Kirshner, R.P., and Oke, J.B. 1975, Ap. J. 200:574.Google Scholar
Lamers, H.J., De Groot, M., and Cassatella, A. 1983, Astron. and Ap. 123:L8.Google Scholar
Langanke, K. and Koonin, S.E. 1983, Nucl. Phys. A. 410:334.Google Scholar
Langanke, K. and Koonin, S.E. 1985, Nucl. Phys. A. In press.Google Scholar
Maeder, A. 1984, Observational Tests of Stellar Evolution Theory, ed. Maeder, A. and Renzini, A., IAU Symp. 105. D. Reidel: Dordrecht, p. 299.Google Scholar
Massey, P. 1981, Ap. J. 246:153.CrossRefGoogle Scholar
Mayle, R. 1985, Ph.D. thesis, UC Berkeley.Google Scholar
Maza, J., and van den Bergh, S. 1976, Ap. J. 204:519.Google Scholar
Mazurek, T.J., Truran, J.W., and Cameron, A.G.W. 1974, Ap. Space Sci. 27:261.Google Scholar
Mazurek, T.J., Meier, D.L., and Wheeler, J.C. 1977, Ap. J. 213:518.Google Scholar
Mazurek, T., Colgate, S.A., and Buchler, J.R. 1980, Jour. de Physique Colloque. C2:159.Google Scholar
Meyerott, R.E. 1980, Ap. J. 239:257.CrossRefGoogle Scholar
Müller, E., and Arnett, W.D. 1982, Ap. J. Lett. 261:L109.Google Scholar
Müller, E., and Arnett, W.D. 1985, Ap. J., in press.Google Scholar
Nomoto, K. 1982a, Ap. J. 253:798.CrossRefGoogle Scholar
Nomoto, K. 1982b. Ap. J. 257:780.CrossRefGoogle Scholar
Nomoto, K. 1984a, Ap. J. 277:791.Google Scholar
Nomoto, K. 1984b, The Crab Nebula and Related Supernova Remnants, ed. Kafatos, M. and Henry, R.B.C., Cambridge Univ. Press: Cambridge. In press.Google Scholar
Nomoto, K. 1985, Proceedings of the 12th Texas Symposium on Relativistic Astrophysics, Ann. N. Y. Acad. Sci., in press.Google Scholar
Nomoto, K., Thielemann, F.-K., and Yokoi, K. 1984, Ap. J. 286:644.Google Scholar
Oemler, A., and Tinsley, B.M. 1979, Astron. J. 84:985.Google Scholar
Pankey, T. 1962, Ph.D. Thesis Howard Univ., Diss. abstr. 23:4.Google Scholar
Pinto, P.A., and Axelrod, T.S. 1986, in preparation for Ap. J.Google Scholar
Romanishin, W., and Angel, J.R.P. 1980, Ap. J. 235:992.CrossRefGoogle Scholar
Schild, R., and Maeder, A. 1983, Astron, and Ap. 130:237.Google Scholar
Sugimoto, D., and Nomoto, K. 1980, Space Sci. Rev. 25:155.Google Scholar
Tammann, G.A. 1974, in Supernovae and Supernova Remnants ed. Cosmovici, C.B.. D. Reidel: Dordrecht, p. 155.Google Scholar
Tammann, G.A. 1982, Supernovae: A Survey of Current Research, ed. Rees, M.J. and Stoneham, R.J. D. Reidel: Dordrecht, p. 371.Google Scholar
Thielemann, F.-K., Nomoto, K., and Yokoi, K. 1985, Astron, and Ap., in press.Google Scholar
Truran, J.W., Arnett, D., and Cameron, A.G.W. 1967, Canadian J. Phys. 45:2315.Google Scholar
Tuchman, Y., Sack, N., and Barkat, Z. 1979, Ap. J. 234:217.Google Scholar
Utrobin, V.P. 1984, Ap. and Spac. Sci. 98:115.Google Scholar
Weaver, T.A., Axelrod, T.S., and Woosley, S.E. 1980, Type I Supernovae, ed. Wheeler, J.C.. Austin: Univ. of Texas, p. 113.Google Scholar
Weaver, T.A., Zimmerman, G.B., and Woosley, S.E., 1978, Ap. J. 225:1021.Google Scholar
Weaver, T.A., Woosley, S.E., and Fuller, G.M. 1985, Numerical Astrophysics, ed. Centrella, J., LeBlanc, J., and Bowers Jones, R. and Bartlett, : Boston, p. 374.Google Scholar
Webbink, R.F. 1984, Ap. J. 277:355.Google Scholar
Weidemann, V., and Koester, D. 1983, Astron, and Ap. 121:77.Google Scholar
Wilson, J.R. 1985a, Numerical Astrophysics, ed. Centrella, J.M., LeBlanc, J.M., and Bowers, R.L., (Jones and Bartlett: Boston), p. 422.Google Scholar
Wilson, J.R. 1985b, private communication.Google Scholar
Wilson, J.R., Mayle, R., Woosley, S.E., and Weaver, T.A. 1985, Proc. of Twelfth Texas Symp. on Rel. Ap., Ann. N. Y. Acad. Sci., in press.Google Scholar
Woosley, S.E., Axelrod, R.S., and Weaver, T.A. 1984, Stellar Nucleosynthesis, ed. Chiosi, C. and Renzini, A., (D. Reidel: Dordrecht), p. 263.CrossRefGoogle Scholar
Woosley, S.E., and Weaver, T.A. 1982a, Supernovae: A Survey of Current Research, ed. Rees, M.J. and Stoneham, R.J., D. Reidel: Dordrecht, p. 79.Google Scholar
Woosley, S.E., and Weaver, T.A. 1982b, Essays in Nuclear Astrophysics, eds. Barnes, C.A., Clayton, D.D., and Schramm, D.N., Cambridge Univ. Press: Cambridge, p. 377.Google Scholar
Woosley, S.E., and Weaver, T.A. 1985, Nucleosynthesis and Its Implications On Nuclear and Particle Physics, Proc. Fifth Moriand Astrohysics Conference, ed. Audouze, J. and van Thuan, T., D. Reidel: Dordrecht, in press.Google Scholar
Woosley, S.E., and Weaver, T.A. 1986a, Ann. Rev. Astron, and Ap., in press.Google Scholar
Woosley, S.E., and Weaver, T.A. 1986b, in preparation for Ap. J.Google Scholar
Woosley, S.E., Weaver, T.A., and Taam, R.E. 1980, Type I Supernovae, ed. Wheeler, J.C., Austin: Univ. of Texas, p. 96.Google Scholar
Woosley, S.E., Taam, R.E., and Weaver, T.A. 1986, Ap. J., 301:000.Google Scholar
Wu, C.-C., Leventhal, M., Sarazin, C.L., and Gull, T.R. 1983, Ap. J. Lett. 269:L5.Google Scholar
Zeldovich, Ya.B., Barenblatt, G.I., Librovich, V.B., and Makhviladze, G.M. 1985, The Mathematical Theory of Combustion and Explosions, Plenum Publ. Corp.: New York.Google Scholar