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Heating of nuclei with energetic antiprotons

Authors :
W. Kurcewicz
J. Galin
B. M. Quednau
Guntram Pausch
P. Figuera
L. Pienkowski
P. Ziem
S. Proschitzki
K. Gulda
S. Schmid
W. Bohne
T.v. Egidy
H. Rossner
H. Fuchs
U. Jahnke
Ye. S. Golubeva
Frank Goldenbaum
W. Schmid
D. Hilscher
D. Polster
John Eades
A. Péghaire
B. Lott
Jerzy Jastrzębski
A. S. Iljinov
M. Morjean
Grand Accélérateur National d'Ions Lourds (GANIL)
Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)
Institut de Physique Nucléaire d'Orsay (IPNO)
Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Source :
Scopus-Elsevier, Physical Review Letters, Physical Review Letters, American Physical Society, 1996, 77, pp.1230-1233. ⟨10.1103/PhysRevLett.77.1230⟩, Physical Review Letters, 1996, 77, pp.1230-1233. ⟨10.1103/PhysRevLett.77.1230⟩

Abstract

The annihilation of energetic (1.2 GeV) antiprotons is exploited to deposit maximum thermal excitation (up to 1000 MeV) in massive nuclei (Cu, Ho, Au, and U) while minimizing the contribution from collective excitation such as rotation, shape distortion, and compression. Excitation energy distributions {ital d}{sigma}/{ital dE}{asterisk} are deduced from eventwise observation of the whole nuclear evaporation chain with two 4{pi} detectors for neutrons and charged particles. The nuclei produced in this way are found to decay predominantly statistically, i.e., by evaporation. {copyright} {ital 1996 The American Physical Society.}

Details

ISSN :
00319007 and 10797114
Database :
OpenAIRE
Journal :
Scopus-Elsevier, Physical Review Letters, Physical Review Letters, American Physical Society, 1996, 77, pp.1230-1233. ⟨10.1103/PhysRevLett.77.1230⟩, Physical Review Letters, 1996, 77, pp.1230-1233. ⟨10.1103/PhysRevLett.77.1230⟩
Accession number :
edsair.doi.dedup.....e3716fc68a60edf3d2e48bece3d796bc
Full Text :
https://doi.org/10.1103/PhysRevLett.77.1230⟩