{ "id": "astro-ph/0110079", "version": "v1", "published": "2001-10-03T13:47:48.000Z", "updated": "2001-10-03T13:47:48.000Z", "title": "Gamma-Ray Signatures of Supernovae and Hypernovae", "authors": [ "K. Nomoto", "K. Maeda", "Y. Mochizuki", "S. Kumagai", "H. Umeda", "T. Nakamura", "I. Tanihata" ], "comment": "Invited talk at the ``GAMMA2001'' Symposium, April 4-6, 2001, Baltimore. To be published in ``Gamma-Ray Astronomy 2001'' (American Institute of Physics)", "doi": "10.1063/1.1419452", "categories": [ "astro-ph" ], "abstract": "We review the characteristics of nucleosynthesis and radioactivities in 'Hypernovae', i.e., supernovae with very large explosion energies ($ \\gsim 10^{52} $ ergs) and their $\\gamma$-ray line signatures. We also discuss the $^{44}$Ti line $\\gamma$-rays from SN1987A and the detectability with INTEGRAL. Signatures of hypernova nucleosynthesis are seen in the large [(Ti, Zn)/Fe] ratios in very metal poor stars. Radioactivities in hypernovae compared to those of ordinary core-collapse supernovae show the following characteristics: 1) The complete Si burning region is more extended, so that the ejected mass of $^{56}$Ni can be much larger. 2) Si-burning takes place in higher entropy and more $\\alpha$-rich environment. Thus the $^{44}$Ti abundance relative to $^{56}$Ni is much larger. In aspherical explosions, $^{44}$Ti is even more abundant and ejected with velocities as high as $\\sim$ 15,000 km s$^{-1}$, which could be observed in $\\gamma$-ray line profiles. 3) The abundance of $^{26}$Al is not so sensitive to the explosion energy, while the $^{60}$Fe abundance is enhanced by a factor of $\\sim$ 3.", "revisions": [ { "version": "v1", "updated": "2001-10-03T13:47:48.000Z" } ], "analyses": { "subjects": [ "95.55.Qf", "97.60.Bw", "26.30.+k", "98.70.Rz" ], "keywords": [ "gamma-ray signatures", "explosion energy", "large explosion energies", "ray line profiles", "ray line signatures" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 577144, "adsabs": "2001AIPC..587..487N" } } }