Reactions Induced by Real Photons for Nuclear Structure and Nuclear Astrophysics

نویسندگان

چکیده

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Probing Nuclear Structure and Nuclear Astrophysics with Real Photons

Examples for recent studies of magnetic dipole and electric quadrupole excitations with the nuclear resonance fluorescence technique at the superconducting Darmstadt electron linear accelerator S–DALINAC are given. The properties of the gross and fine structure of the orbital magnetic scissors mode in even and odd-mass nuclei are summarized. Within a test experiment, the decay width of the exci...

متن کامل

NUSTAR-T Theoretical Nuclear Structure, Astrophysics and Reactions

NUSTAR-T-05 Effective nuclear forces and low lying collective excitations in Sn 109 NUSTAR-T-07 Relativistic quasiparticle RPA with applications to exotic nuclei 111

متن کامل

Direct Reactions with Exotic Nuclei , Nuclear Structure and Astrophysics

Intermediate energy Coulomb excitation and dissociation is a useful tool for nuclear structure and astrophysics studies. Low-lying strength in nuclei far from stability was discovered by this method. The effective range theory for low-lying strength in one-neutron halo nuclei is summarized and extended to two-neutron halo nuclei. This is of special interest in view of recent rather accurate exp...

متن کامل

Nuclear Structure and Nuclear Reactions

Atomic nuclei are the essence of the visible universe. Formed in the big bang or in cataclysmic astrophysical explosions, atomic nuclei are a crucial and intriguing part of the world. The basic features of atomic nuclei were understood in terms of the nuclear shell model in the 1963 Nobel Prize winning research of Eugene Paul Wigner, Maria Goeppert-Mayer, and J. Hans de Jensen. Since then, exte...

متن کامل

Dense Plasmas, Nuclear Reactions and Astrophysics

A certain number of questions are raised to physicists and astrophysicists concerning : (1) the conditions under which stellar matter becomes a highly correlated plasma ; (2) the role of mass loss in the formation of dense matter ; (3) the evolution of white dwarfs accreting matter (with its consequences for the formation of compact X ray sources and pulsars) . 1 . Introduction.The solution of ...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Physics Procedia

سال: 2012

ISSN: 1875-3892

DOI: 10.1016/j.phpro.2012.04.015