The rp-process in x-ray bursts

被引:0
|
作者
Wiescher, M [1 ]
Aprahamian, A [1 ]
Döring, J [1 ]
Görres, J [1 ]
机构
[1] Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA
来源
NUCLEAR STRUCTURE 98 | 1999年 / 481卷
关键词
D O I
暂无
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
The rp-process was first suggested by Wallace and Woosley (1981) as the dominant nucleosynthesis process in explosive hydrogen burning at high temperature and density conditions. The process is characterized by a sequence of fast proton capture reactions and subsequent beta-decays. The reaction path of the rp-process runs along the drip line up to Z approximate to 50. Within a sufficiently long time scale for the thermonuclear runaway mainly N=Z even-even nuclei are produced in the associated nucleosynthesis. Extended model calculations indicate a large production of mass A=80 isotopes. The resulting abundances are extremely sensitiveto the structure, lifetimes and decay pattern of the relevant isotopes. Experimental results are presented here for Zr-80 along with a discussion of the associated nucleosynthesis.
引用
收藏
页码:545 / 553
页数:9
相关论文
共 50 条
  • [1] The rp-process in X-ray bursts
    Schatz, H
    Bildsten, L
    Gorres, J
    Wiescher, M
    Thielemann, FK
    INTERSECTIONS BETWEEN PARTICLE AND NUCLEAR PHYSICS - 6TH CONFERENCE, 1997, (412): : 987 - 991
  • [2] The rp-process in X-ray bursts
    Wiescher, M
    Aprahamian, A
    Döring, J
    Görres, J
    Schatz, H
    ENAM 98: EXOTIC NUCLEI AND ATOMIC MASSES, 1998, 455 : 819 - 826
  • [3] Explosive H-burning, the rp-process, and X-ray bursts
    Thielemann, FK
    Schatz, H
    Rauscher, T
    Rembges, JF
    Gorres, J
    Wiescher, M
    Bildsten, L
    STELLAR EVOLUTION, STELLAR EXPLOSIONS AND GALACTIC CHEMICAL EVOLUTION, 1998, : 483 - 494
  • [4] The rp-process at X-ray burst conditions
    Wiescher, M
    Schatz, H
    INTERSECTIONS OF PARTICLE AND NUCLEAR PHYSICS, 2000, 549 : 744 - 750
  • [5] Rare isotopes and accreting neutron stars, X-ray bursts, neutron star crust, rp-process
    Schatz, H.
    EXOTIC NUCLEI AND NUCLEAR /PARTICLE ASTROPHYSICS (II), 2008, 972 : 309 - 317
  • [6] Beta decay along the N=Z line and its relevance in rp-process and X-Ray bursts
    Nacher, E.
    Parra, S.
    Briz, J. A.
    Aguilera, P.
    Agramunt, J.
    Algora, A.
    Berry, T.
    Borge, M. J. G.
    Carmona, M.
    Fraile, L. M.
    Ganioglu, E.
    Gelletly, W.
    Guadilla, V.
    Illana, A.
    Lica, R.
    Marroquin, I.
    Molina, F.
    Morales, A. I.
    Orce, N.
    Orrigo, S. E. J.
    Perea, A.
    Romero, J.
    Rubio, B.
    Sotty, C.
    Tain, J. L.
    Tengblad, O.
    Tolosa, A.
    NUCLEAR PHYSICS IN ASTROPHYSICS - X, NPA-X 2022, 2023, 279
  • [7] Models of Type I X-ray bursts from GS 1826-24: a probe of rp-process hydrogen burning
    Heger, Alexander
    Cumming, Andrew
    Galloway, Duncan K.
    Woosley, Stanford E.
    ASTROPHYSICAL JOURNAL LETTERS, 2007, 671 (02) : L141 - L144
  • [9] Neutron star cooling and the rp process in thermonuclear X-ray bursts
    in't Zand, J. J. M.
    Visser, M. E. B.
    Galloway, D. K.
    Chenevez, J.
    Keek, L.
    Kuulkers, E.
    Sanchez-Fernandez, C.
    Woerpel, H.
    ASTRONOMY & ASTROPHYSICS, 2017, 606
  • [10] Consistent Modeling of GS 1826-24 X-Ray Bursts for Multiple Accretion Rates Demonstrates the Possibility of Constraining rp-process Reaction Rates
    Meisel, Zach
    ASTROPHYSICAL JOURNAL, 2018, 860 (02):