Predicted cross-sections for photon-induced particle emission

T. Rauscher; Friedrich-Karl Thielemann

doi:10.1016/j.adt.2004.07.001

Predicted cross-sections for photon-induced particle emission

T. Rauscher, Friedrich-Karl Thielemann

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Abstract

Cross-sections for the photon-induced particle-emission reactions (gamma,n), (gamma,p), and (gamma,alpha) are given for all natural isotopes from Ti to Bi. The target nuclei are assumed to be in their ground states, except for Ta-180 which is naturally occurring as the isomer Ta-180m. The cross-sections are calculated in a statistical model (Hauser-Feshbach) approach and covering an energy range from threshold up to 7.35 MeV above the threshold (14.7 MeV above threshold for (gamma,alpha) reactions). The results are intended to aid conception and analysis of experiments which can also be used to test the methods involved in predicting astrophysical reaction rates for nucleo-synthesis. (C) 2004 Elsevier Inc. All rights reserved.

Original language	English
Pages (from-to)	1-81
Number of pages	81
Journal	Atomic Data and Nuclear Data Tables
Volume	88
Issue number	1
DOIs	https://doi.org/10.1016/j.adt.2004.07.001
Publication status	Published - Sept 2004

Keywords

GAMMA-PROCESS
STATISTICAL-MODEL CALCULATIONS
BREMSSTRAHLUNG
HEAVY-ELEMENTS
ASTROPHYSICAL REACTION-RATES
S-PROCESS
NUCLEOSYNTHESIS
NUCLEAR ASTROPHYSICS

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title = "Predicted cross-sections for photon-induced particle emission",

abstract = "Cross-sections for the photon-induced particle-emission reactions (gamma,n), (gamma,p), and (gamma,alpha) are given for all natural isotopes from Ti to Bi. The target nuclei are assumed to be in their ground states, except for Ta-180 which is naturally occurring as the isomer Ta-180m. The cross-sections are calculated in a statistical model (Hauser-Feshbach) approach and covering an energy range from threshold up to 7.35 MeV above the threshold (14.7 MeV above threshold for (gamma,alpha) reactions). The results are intended to aid conception and analysis of experiments which can also be used to test the methods involved in predicting astrophysical reaction rates for nucleo-synthesis. (C) 2004 Elsevier Inc. All rights reserved.",

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author = "T. Rauscher and Friedrich-Karl Thielemann",

year = "2004",

month = sep,

doi = "10.1016/j.adt.2004.07.001",

language = "English",

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journal = "Atomic Data and Nuclear Data Tables",

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T1 - Predicted cross-sections for photon-induced particle emission

AU - Rauscher, T.

AU - Thielemann, Friedrich-Karl

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N2 - Cross-sections for the photon-induced particle-emission reactions (gamma,n), (gamma,p), and (gamma,alpha) are given for all natural isotopes from Ti to Bi. The target nuclei are assumed to be in their ground states, except for Ta-180 which is naturally occurring as the isomer Ta-180m. The cross-sections are calculated in a statistical model (Hauser-Feshbach) approach and covering an energy range from threshold up to 7.35 MeV above the threshold (14.7 MeV above threshold for (gamma,alpha) reactions). The results are intended to aid conception and analysis of experiments which can also be used to test the methods involved in predicting astrophysical reaction rates for nucleo-synthesis. (C) 2004 Elsevier Inc. All rights reserved.

AB - Cross-sections for the photon-induced particle-emission reactions (gamma,n), (gamma,p), and (gamma,alpha) are given for all natural isotopes from Ti to Bi. The target nuclei are assumed to be in their ground states, except for Ta-180 which is naturally occurring as the isomer Ta-180m. The cross-sections are calculated in a statistical model (Hauser-Feshbach) approach and covering an energy range from threshold up to 7.35 MeV above the threshold (14.7 MeV above threshold for (gamma,alpha) reactions). The results are intended to aid conception and analysis of experiments which can also be used to test the methods involved in predicting astrophysical reaction rates for nucleo-synthesis. (C) 2004 Elsevier Inc. All rights reserved.

KW - GAMMA-PROCESS

KW - STATISTICAL-MODEL CALCULATIONS

KW - BREMSSTRAHLUNG

KW - HEAVY-ELEMENTS

KW - ASTROPHYSICAL REACTION-RATES

KW - S-PROCESS

KW - NUCLEOSYNTHESIS

KW - NUCLEAR ASTROPHYSICS

U2 - 10.1016/j.adt.2004.07.001

DO - 10.1016/j.adt.2004.07.001

M3 - Article

SN - 0092-640X

VL - 88

SP - 1

EP - 81

JO - Atomic Data and Nuclear Data Tables

JF - Atomic Data and Nuclear Data Tables

IS - 1

ER -

Predicted cross-sections for photon-induced particle emission

Abstract

Keywords

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