1973
DOI: 10.1086/190271
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Partial Cross-Sections in High-Energy Nuclear Reactions, and Astrophysical Applications. I. Targets WITh Z <= 28. II. Targets Heavier than Nickel

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Cited by 376 publications
(130 citation statements)
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“…As pointed out above there is no adequate model describing proton-induced high-energy reactions. Several attempts have been made to describe the cross sections of high-energy reactions by semiempirical formulae [41,42,43,44]. The formulae by Rudstam [41] and Silberberg and Tsao [42] tumed out to be widely unreliable and only to represent the general trends of high-energy cross sections.…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…As pointed out above there is no adequate model describing proton-induced high-energy reactions. Several attempts have been made to describe the cross sections of high-energy reactions by semiempirical formulae [41,42,43,44]. The formulae by Rudstam [41] and Silberberg and Tsao [42] tumed out to be widely unreliable and only to represent the general trends of high-energy cross sections.…”
Section: Discussionmentioning
confidence: 99%
“…Several attempts have been made to describe the cross sections of high-energy reactions by semiempirical formulae [41,42,43,44]. The formulae by Rudstam [41] and Silberberg and Tsao [42] tumed out to be widely unreliable and only to represent the general trends of high-energy cross sections. It is not clear up to now, whether the deficits of these approaches are due to these authors using an at that time insufficient data base.…”
Section: Discussionmentioning
confidence: 99%
“…Nuclei injected at earlier times should suffer significant fragmentation in collisions with the matter inside the nebula. We have simulated this process of fragmentation of nuclei injected by the pulsar applying the semiempirical formulae for the cross sections for the fragmentation of nuclei of Silberberg & Tsao [47] with parameters given in their tables 1A,B,C,D. In our simulation, we assumed that in a single collision a nucleus fragments into two nuclei with different mass numbers.…”
Section: Interaction Of Nuclei With Matter Inside Nebulaementioning
confidence: 99%
“…Twelve detectors were located at a distance of 38 cm from the centre of the target at angles from 10°, to 150° with respect to the incident beam. The spallation reactions used are shown in Table 1. The energy dependent spallation reaction cross-sections were calculated using the semiempirical cross-section formulae of Rudstam [6] or Silberberg and Tsao [7]. The Silberberg-Tsao formulae were used only for the Cu - 7 Be cross-section calculations where the Rudstam formulae are not applicable.…”
Section: Hadron Fluence Spectramentioning
confidence: 99%
“…The spallation reactions used are shown in Table 1. The energy dependent spallation reaction cross-sections were calculated using the semiempirical cross-section formulae of Rudstam [6] or Silberberg and Tsao [7]. The Silberberg-Tsao formulae were used only for the Cu - 7 Be cross-section calculations where the Rudstam formulae are not applicable. The effective cross-section was calculated from the energy dependent cross-sections using a constant weighting spectrum which is justified when the cross-sections have a clear threshold behaviour.…”
Section: Hadron Fluence Spectramentioning
confidence: 99%