University of Hertfordshire Research Archive

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        AuthorRauscher, T. (54)Heil, M. (19)Abbondanno, U. (17)Aerts, G. (17)Alvarez-Velarde, F. (17)Andrzejewski, J. (17)Baumann, P. (17)Calvino, F. (17)Cano-Ott, D. (17)Capote, R. (17)... View MoreDate Issued2010 - 2014 (14)2000 - 2009 (37)1994 - 1999 (5)SchoolSchool of Physics, Astronomy and Mathematics (56)

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        Capture of a particles by isospin-symmetric nuclei 

        Rauscher, T.; Thielemann, Friedrich-Karl; Gorres, J.; Wiescher, M. (2000-08-14)
        The reaction rates for ct capture processes on self-conjugate nuclei in the mass range A = 20-40 have been investigated. The rates were calculated using the statistical model code NON-SMOKER taking into account isospin ...

        Low-metallicity inhibition of type Ia supernovae and galactic and cosmic chemical evolution 

        Kobayashi, Chiaki; Tsujimoto, T; Nomoto, K; Hachisu, I; Kato, M (1998-08-20)
        We introduce a metallicity dependence of the Type Ia supernova (SN Ia) rate into the Galactic and cosmic chemical evolution models. In our SN Ia progenitor scenario, the accreting white dwarf (WD) blows a strong wind to ...

        First beta-decay studies of the neutron-rich isotopes Sc53-55 and V56-59 

        Sorlin, O.; Borrel, V.; Grevy, S.; Guillemaud-Mueller, D.; Mueller, A.C.; Pougheon, F.; Bohmer, W.; Kratz, K.L.; Mehren, T.; Moller, P.; Pfeiffer, B.; Rauscher, T.; Saint-Laurent, M.G.; Anne, R.; Lewitowicz, M.; Ostrowski, A.; Dorfler, T.; Schmidt-Ott, W.D. (1998-03-16)
        The neutron-rich isotopes Sc53-55 and V56-59 have been produced at GANIL in interactions of a 64.5 MeV/u Cu-65 beam with a Be-9 target. They were separated by the doubly achromatic spectrometer LISE3. Beta-decay half-lives ...

        The r-process in the high entropy bubble 

        Freiburghaus, C.; Rauscher, T.; Thielemann, Friedrich-Karl; Kratz, K.L.; Pfeiffer, B. (1997-08-04)

        An approximation for the rp-process 

        Rembges, F.; Freiburghaus, C.; Rauscher, T.; Thielemann, F.K.; Schatz, H.; Wiescher, M. (1997-07-20)
        Hot (explosive) hydrogen burning, or the rapid proton capture process (rp-process), occurs in a number of astrophysical environments. Novae and X-ray bursts are the most prominent ones, but accretion disks around black ...

        Astrophysics and nuclei far from stabilitys 

        Thielemann, F.K.; Kratz, K.L.; Pfeiffer, B.; Rauscher, T.; van Wormer, L.; Wiescher, M. (1994-03)
        We discuss unstable nuclei on the proton-rich and neutron rich side of stability and their properties of astrophysical relevance. The Coulomb barriers in charged-particle captures lead to a cycle pattern which is not ...
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