Chromium and titanium isotopes produced in photonuclear reactions of vanadium, revisited
Photonuclear production yields of ^5^1Ti und ^5^1^,^4^9^,^4^8Cr from ^5^1V were redetermined for bremsstrahlung end-point energies (E"0) of 30 to 1000 or 1050 MeV with the aid of radiochemical separation of Cr. The yield curves for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr show a clear evidence for two...
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E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1989 |
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| Reproduktion: |
Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 |
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| Übergeordnetes Werk: |
in: Nuclear Physics, Section A - Amsterdam : Elsevier, 501(1989), 4, Seite 693-709 |
| Übergeordnetes Werk: |
volume:501 ; year:1989 ; number:4 ; pages:693-709 |
| Links: |
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NLEJ181209381 |
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| 245 | 1 | 0 | |a Chromium and titanium isotopes produced in photonuclear reactions of vanadium, revisited |
| 264 | 1 | |c 1989 | |
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| 520 | |a Photonuclear production yields of ^5^1Ti und ^5^1^,^4^9^,^4^8Cr from ^5^1V were redetermined for bremsstrahlung end-point energies (E"0) of 30 to 1000 or 1050 MeV with the aid of radiochemical separation of Cr. The yield curves for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr show a clear evidence for two components in the production process; one tor secondary-proton reactions at E"0 < Q"π and the other for photopion reactions, at E"0 > Q, Q"π being Q-values for (γ, π^+) and (γ, π^+ xn) reactions. The contributions of the secondary reactions for production of the Ti and Cr isotopes at E"0 > Q"π were then estimated by fitting calculated secondary yields to the observed ones at E"0 < Q"π, and found to be about 40%, 20%, 4% and 4% for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr, respectively, at E"0 = 400 to 1000 MeV. The calculation of the secondary yields was based on the excitation functions for ^5^1V(n, p) and (p, x'n) calculated with the ALICE code and the reported photoneutron and photoproton spectra from ^1^2C and some other complex nuclei.The present results for ^4^9Cr are close to the reported ones, while the present ^4^8Cr yields differ by a factor of about 50. For the ^5^1Ti and ^5^1Cr yields, there are some discrepancies between the present and reported ones. The yield corrected for the secondaries, in units of μb/equivalent quantum, were unfolded into cross sections per photon, in units of μb, as a function ol monochromatic photon energy with the LOUHI-82 code. The results for the ^5^1Ti and ^4^9Cr are in disagreement in both the magnitude and shape with the theoretical predictions based on DWIA and PWIA. A Monte Carlo calculation based on the PICA code by Gabriel and Alsmiller does reproduce the gross feature of the present results. | ||
| 533 | |f Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 | ||
| 700 | 1 | |a Sakamoto, K. |4 oth | |
| 700 | 1 | |a Yoshida, M. |4 oth | |
| 700 | 1 | |a Kubota, Y. |4 oth | |
| 700 | 1 | |a Fukasawa, T. |4 oth | |
| 700 | 1 | |a Kunugise, A. |4 oth | |
| 700 | 1 | |a Hamajima, Y. |4 oth | |
| 700 | 1 | |a Shibata, S. |4 oth | |
| 700 | 1 | |a Fujiwara, I. |4 oth | |
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(DE-627)NLEJ181209381 (DE-599)GBVNLZ181209381 DE-627 ger DE-627 rakwb eng Chromium and titanium isotopes produced in photonuclear reactions of vanadium, revisited 1989 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Photonuclear production yields of ^5^1Ti und ^5^1^,^4^9^,^4^8Cr from ^5^1V were redetermined for bremsstrahlung end-point energies (E"0) of 30 to 1000 or 1050 MeV with the aid of radiochemical separation of Cr. The yield curves for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr show a clear evidence for two components in the production process; one tor secondary-proton reactions at E"0 < Q"π and the other for photopion reactions, at E"0 > Q, Q"π being Q-values for (γ, π^+) and (γ, π^+ xn) reactions. The contributions of the secondary reactions for production of the Ti and Cr isotopes at E"0 > Q"π were then estimated by fitting calculated secondary yields to the observed ones at E"0 < Q"π, and found to be about 40%, 20%, 4% and 4% for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr, respectively, at E"0 = 400 to 1000 MeV. The calculation of the secondary yields was based on the excitation functions for ^5^1V(n, p) and (p, x'n) calculated with the ALICE code and the reported photoneutron and photoproton spectra from ^1^2C and some other complex nuclei.The present results for ^4^9Cr are close to the reported ones, while the present ^4^8Cr yields differ by a factor of about 50. For the ^5^1Ti and ^5^1Cr yields, there are some discrepancies between the present and reported ones. The yield corrected for the secondaries, in units of μb/equivalent quantum, were unfolded into cross sections per photon, in units of μb, as a function ol monochromatic photon energy with the LOUHI-82 code. The results for the ^5^1Ti and ^4^9Cr are in disagreement in both the magnitude and shape with the theoretical predictions based on DWIA and PWIA. A Monte Carlo calculation based on the PICA code by Gabriel and Alsmiller does reproduce the gross feature of the present results. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Sakamoto, K. oth Yoshida, M. oth Kubota, Y. oth Fukasawa, T. oth Kunugise, A. oth Hamajima, Y. oth Shibata, S. oth Fujiwara, I. oth in Nuclear Physics, Section A Amsterdam : Elsevier 501(1989), 4, Seite 693-709 (DE-627)NLEJ177217928 (DE-600)1466542-6 0375-9474 nnns volume:501 year:1989 number:4 pages:693-709 http://linkinghub.elsevier.com/retrieve/pii/0375-9474(89)90156-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 501 1989 4 693-709 |
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(DE-627)NLEJ181209381 (DE-599)GBVNLZ181209381 DE-627 ger DE-627 rakwb eng Chromium and titanium isotopes produced in photonuclear reactions of vanadium, revisited 1989 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Photonuclear production yields of ^5^1Ti und ^5^1^,^4^9^,^4^8Cr from ^5^1V were redetermined for bremsstrahlung end-point energies (E"0) of 30 to 1000 or 1050 MeV with the aid of radiochemical separation of Cr. The yield curves for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr show a clear evidence for two components in the production process; one tor secondary-proton reactions at E"0 < Q"π and the other for photopion reactions, at E"0 > Q, Q"π being Q-values for (γ, π^+) and (γ, π^+ xn) reactions. The contributions of the secondary reactions for production of the Ti and Cr isotopes at E"0 > Q"π were then estimated by fitting calculated secondary yields to the observed ones at E"0 < Q"π, and found to be about 40%, 20%, 4% and 4% for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr, respectively, at E"0 = 400 to 1000 MeV. The calculation of the secondary yields was based on the excitation functions for ^5^1V(n, p) and (p, x'n) calculated with the ALICE code and the reported photoneutron and photoproton spectra from ^1^2C and some other complex nuclei.The present results for ^4^9Cr are close to the reported ones, while the present ^4^8Cr yields differ by a factor of about 50. For the ^5^1Ti and ^5^1Cr yields, there are some discrepancies between the present and reported ones. The yield corrected for the secondaries, in units of μb/equivalent quantum, were unfolded into cross sections per photon, in units of μb, as a function ol monochromatic photon energy with the LOUHI-82 code. The results for the ^5^1Ti and ^4^9Cr are in disagreement in both the magnitude and shape with the theoretical predictions based on DWIA and PWIA. A Monte Carlo calculation based on the PICA code by Gabriel and Alsmiller does reproduce the gross feature of the present results. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Sakamoto, K. oth Yoshida, M. oth Kubota, Y. oth Fukasawa, T. oth Kunugise, A. oth Hamajima, Y. oth Shibata, S. oth Fujiwara, I. oth in Nuclear Physics, Section A Amsterdam : Elsevier 501(1989), 4, Seite 693-709 (DE-627)NLEJ177217928 (DE-600)1466542-6 0375-9474 nnns volume:501 year:1989 number:4 pages:693-709 http://linkinghub.elsevier.com/retrieve/pii/0375-9474(89)90156-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 501 1989 4 693-709 |
| allfields_unstemmed |
(DE-627)NLEJ181209381 (DE-599)GBVNLZ181209381 DE-627 ger DE-627 rakwb eng Chromium and titanium isotopes produced in photonuclear reactions of vanadium, revisited 1989 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Photonuclear production yields of ^5^1Ti und ^5^1^,^4^9^,^4^8Cr from ^5^1V were redetermined for bremsstrahlung end-point energies (E"0) of 30 to 1000 or 1050 MeV with the aid of radiochemical separation of Cr. The yield curves for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr show a clear evidence for two components in the production process; one tor secondary-proton reactions at E"0 < Q"π and the other for photopion reactions, at E"0 > Q, Q"π being Q-values for (γ, π^+) and (γ, π^+ xn) reactions. The contributions of the secondary reactions for production of the Ti and Cr isotopes at E"0 > Q"π were then estimated by fitting calculated secondary yields to the observed ones at E"0 < Q"π, and found to be about 40%, 20%, 4% and 4% for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr, respectively, at E"0 = 400 to 1000 MeV. The calculation of the secondary yields was based on the excitation functions for ^5^1V(n, p) and (p, x'n) calculated with the ALICE code and the reported photoneutron and photoproton spectra from ^1^2C and some other complex nuclei.The present results for ^4^9Cr are close to the reported ones, while the present ^4^8Cr yields differ by a factor of about 50. For the ^5^1Ti and ^5^1Cr yields, there are some discrepancies between the present and reported ones. The yield corrected for the secondaries, in units of μb/equivalent quantum, were unfolded into cross sections per photon, in units of μb, as a function ol monochromatic photon energy with the LOUHI-82 code. The results for the ^5^1Ti and ^4^9Cr are in disagreement in both the magnitude and shape with the theoretical predictions based on DWIA and PWIA. A Monte Carlo calculation based on the PICA code by Gabriel and Alsmiller does reproduce the gross feature of the present results. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Sakamoto, K. oth Yoshida, M. oth Kubota, Y. oth Fukasawa, T. oth Kunugise, A. oth Hamajima, Y. oth Shibata, S. oth Fujiwara, I. oth in Nuclear Physics, Section A Amsterdam : Elsevier 501(1989), 4, Seite 693-709 (DE-627)NLEJ177217928 (DE-600)1466542-6 0375-9474 nnns volume:501 year:1989 number:4 pages:693-709 http://linkinghub.elsevier.com/retrieve/pii/0375-9474(89)90156-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 501 1989 4 693-709 |
| allfieldsGer |
(DE-627)NLEJ181209381 (DE-599)GBVNLZ181209381 DE-627 ger DE-627 rakwb eng Chromium and titanium isotopes produced in photonuclear reactions of vanadium, revisited 1989 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Photonuclear production yields of ^5^1Ti und ^5^1^,^4^9^,^4^8Cr from ^5^1V were redetermined for bremsstrahlung end-point energies (E"0) of 30 to 1000 or 1050 MeV with the aid of radiochemical separation of Cr. The yield curves for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr show a clear evidence for two components in the production process; one tor secondary-proton reactions at E"0 < Q"π and the other for photopion reactions, at E"0 > Q, Q"π being Q-values for (γ, π^+) and (γ, π^+ xn) reactions. The contributions of the secondary reactions for production of the Ti and Cr isotopes at E"0 > Q"π were then estimated by fitting calculated secondary yields to the observed ones at E"0 < Q"π, and found to be about 40%, 20%, 4% and 4% for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr, respectively, at E"0 = 400 to 1000 MeV. The calculation of the secondary yields was based on the excitation functions for ^5^1V(n, p) and (p, x'n) calculated with the ALICE code and the reported photoneutron and photoproton spectra from ^1^2C and some other complex nuclei.The present results for ^4^9Cr are close to the reported ones, while the present ^4^8Cr yields differ by a factor of about 50. For the ^5^1Ti and ^5^1Cr yields, there are some discrepancies between the present and reported ones. The yield corrected for the secondaries, in units of μb/equivalent quantum, were unfolded into cross sections per photon, in units of μb, as a function ol monochromatic photon energy with the LOUHI-82 code. The results for the ^5^1Ti and ^4^9Cr are in disagreement in both the magnitude and shape with the theoretical predictions based on DWIA and PWIA. A Monte Carlo calculation based on the PICA code by Gabriel and Alsmiller does reproduce the gross feature of the present results. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Sakamoto, K. oth Yoshida, M. oth Kubota, Y. oth Fukasawa, T. oth Kunugise, A. oth Hamajima, Y. oth Shibata, S. oth Fujiwara, I. oth in Nuclear Physics, Section A Amsterdam : Elsevier 501(1989), 4, Seite 693-709 (DE-627)NLEJ177217928 (DE-600)1466542-6 0375-9474 nnns volume:501 year:1989 number:4 pages:693-709 http://linkinghub.elsevier.com/retrieve/pii/0375-9474(89)90156-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 501 1989 4 693-709 |
| allfieldsSound |
(DE-627)NLEJ181209381 (DE-599)GBVNLZ181209381 DE-627 ger DE-627 rakwb eng Chromium and titanium isotopes produced in photonuclear reactions of vanadium, revisited 1989 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Photonuclear production yields of ^5^1Ti und ^5^1^,^4^9^,^4^8Cr from ^5^1V were redetermined for bremsstrahlung end-point energies (E"0) of 30 to 1000 or 1050 MeV with the aid of radiochemical separation of Cr. The yield curves for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr show a clear evidence for two components in the production process; one tor secondary-proton reactions at E"0 < Q"π and the other for photopion reactions, at E"0 > Q, Q"π being Q-values for (γ, π^+) and (γ, π^+ xn) reactions. The contributions of the secondary reactions for production of the Ti and Cr isotopes at E"0 > Q"π were then estimated by fitting calculated secondary yields to the observed ones at E"0 < Q"π, and found to be about 40%, 20%, 4% and 4% for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr, respectively, at E"0 = 400 to 1000 MeV. The calculation of the secondary yields was based on the excitation functions for ^5^1V(n, p) and (p, x'n) calculated with the ALICE code and the reported photoneutron and photoproton spectra from ^1^2C and some other complex nuclei.The present results for ^4^9Cr are close to the reported ones, while the present ^4^8Cr yields differ by a factor of about 50. For the ^5^1Ti and ^5^1Cr yields, there are some discrepancies between the present and reported ones. The yield corrected for the secondaries, in units of μb/equivalent quantum, were unfolded into cross sections per photon, in units of μb, as a function ol monochromatic photon energy with the LOUHI-82 code. The results for the ^5^1Ti and ^4^9Cr are in disagreement in both the magnitude and shape with the theoretical predictions based on DWIA and PWIA. A Monte Carlo calculation based on the PICA code by Gabriel and Alsmiller does reproduce the gross feature of the present results. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Sakamoto, K. oth Yoshida, M. oth Kubota, Y. oth Fukasawa, T. oth Kunugise, A. oth Hamajima, Y. oth Shibata, S. oth Fujiwara, I. oth in Nuclear Physics, Section A Amsterdam : Elsevier 501(1989), 4, Seite 693-709 (DE-627)NLEJ177217928 (DE-600)1466542-6 0375-9474 nnns volume:501 year:1989 number:4 pages:693-709 http://linkinghub.elsevier.com/retrieve/pii/0375-9474(89)90156-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 501 1989 4 693-709 |
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The yield curves for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr show a clear evidence for two components in the production process; one tor secondary-proton reactions at E"0 < Q"π and the other for photopion reactions, at E"0 > Q, Q"π being Q-values for (γ, π^+) and (γ, π^+ xn) reactions. The contributions of the secondary reactions for production of the Ti and Cr isotopes at E"0 > Q"π were then estimated by fitting calculated secondary yields to the observed ones at E"0 < Q"π, and found to be about 40%, 20%, 4% and 4% for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr, respectively, at E"0 = 400 to 1000 MeV. The calculation of the secondary yields was based on the excitation functions for ^5^1V(n, p) and (p, x'n) calculated with the ALICE code and the reported photoneutron and photoproton spectra from ^1^2C and some other complex nuclei.The present results for ^4^9Cr are close to the reported ones, while the present ^4^8Cr yields differ by a factor of about 50. 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Chromium and titanium isotopes produced in photonuclear reactions of vanadium, revisited |
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Chromium and titanium isotopes produced in photonuclear reactions of vanadium, revisited |
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(DE-627)NLEJ181209381 (DE-599)GBVNLZ181209381 |
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Chromium and titanium isotopes produced in photonuclear reactions of vanadium, revisited |
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Nuclear Physics, Section A |
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Nuclear Physics, Section A |
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eng |
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1989 |
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693 |
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501 |
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Elektronische Aufsätze |
| title_sort |
chromium and titanium isotopes produced in photonuclear reactions of vanadium, revisited |
| title_auth |
Chromium and titanium isotopes produced in photonuclear reactions of vanadium, revisited |
| abstract |
Photonuclear production yields of ^5^1Ti und ^5^1^,^4^9^,^4^8Cr from ^5^1V were redetermined for bremsstrahlung end-point energies (E"0) of 30 to 1000 or 1050 MeV with the aid of radiochemical separation of Cr. The yield curves for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr show a clear evidence for two components in the production process; one tor secondary-proton reactions at E"0 < Q"π and the other for photopion reactions, at E"0 > Q, Q"π being Q-values for (γ, π^+) and (γ, π^+ xn) reactions. The contributions of the secondary reactions for production of the Ti and Cr isotopes at E"0 > Q"π were then estimated by fitting calculated secondary yields to the observed ones at E"0 < Q"π, and found to be about 40%, 20%, 4% and 4% for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr, respectively, at E"0 = 400 to 1000 MeV. The calculation of the secondary yields was based on the excitation functions for ^5^1V(n, p) and (p, x'n) calculated with the ALICE code and the reported photoneutron and photoproton spectra from ^1^2C and some other complex nuclei.The present results for ^4^9Cr are close to the reported ones, while the present ^4^8Cr yields differ by a factor of about 50. For the ^5^1Ti and ^5^1Cr yields, there are some discrepancies between the present and reported ones. The yield corrected for the secondaries, in units of μb/equivalent quantum, were unfolded into cross sections per photon, in units of μb, as a function ol monochromatic photon energy with the LOUHI-82 code. The results for the ^5^1Ti and ^4^9Cr are in disagreement in both the magnitude and shape with the theoretical predictions based on DWIA and PWIA. A Monte Carlo calculation based on the PICA code by Gabriel and Alsmiller does reproduce the gross feature of the present results. |
| abstractGer |
Photonuclear production yields of ^5^1Ti und ^5^1^,^4^9^,^4^8Cr from ^5^1V were redetermined for bremsstrahlung end-point energies (E"0) of 30 to 1000 or 1050 MeV with the aid of radiochemical separation of Cr. The yield curves for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr show a clear evidence for two components in the production process; one tor secondary-proton reactions at E"0 < Q"π and the other for photopion reactions, at E"0 > Q, Q"π being Q-values for (γ, π^+) and (γ, π^+ xn) reactions. The contributions of the secondary reactions for production of the Ti and Cr isotopes at E"0 > Q"π were then estimated by fitting calculated secondary yields to the observed ones at E"0 < Q"π, and found to be about 40%, 20%, 4% and 4% for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr, respectively, at E"0 = 400 to 1000 MeV. The calculation of the secondary yields was based on the excitation functions for ^5^1V(n, p) and (p, x'n) calculated with the ALICE code and the reported photoneutron and photoproton spectra from ^1^2C and some other complex nuclei.The present results for ^4^9Cr are close to the reported ones, while the present ^4^8Cr yields differ by a factor of about 50. For the ^5^1Ti and ^5^1Cr yields, there are some discrepancies between the present and reported ones. The yield corrected for the secondaries, in units of μb/equivalent quantum, were unfolded into cross sections per photon, in units of μb, as a function ol monochromatic photon energy with the LOUHI-82 code. The results for the ^5^1Ti and ^4^9Cr are in disagreement in both the magnitude and shape with the theoretical predictions based on DWIA and PWIA. A Monte Carlo calculation based on the PICA code by Gabriel and Alsmiller does reproduce the gross feature of the present results. |
| abstract_unstemmed |
Photonuclear production yields of ^5^1Ti und ^5^1^,^4^9^,^4^8Cr from ^5^1V were redetermined for bremsstrahlung end-point energies (E"0) of 30 to 1000 or 1050 MeV with the aid of radiochemical separation of Cr. The yield curves for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr show a clear evidence for two components in the production process; one tor secondary-proton reactions at E"0 < Q"π and the other for photopion reactions, at E"0 > Q, Q"π being Q-values for (γ, π^+) and (γ, π^+ xn) reactions. The contributions of the secondary reactions for production of the Ti and Cr isotopes at E"0 > Q"π were then estimated by fitting calculated secondary yields to the observed ones at E"0 < Q"π, and found to be about 40%, 20%, 4% and 4% for ^5^1Ti, ^5^1Cr, ^4^9Cr and ^4^8Cr, respectively, at E"0 = 400 to 1000 MeV. The calculation of the secondary yields was based on the excitation functions for ^5^1V(n, p) and (p, x'n) calculated with the ALICE code and the reported photoneutron and photoproton spectra from ^1^2C and some other complex nuclei.The present results for ^4^9Cr are close to the reported ones, while the present ^4^8Cr yields differ by a factor of about 50. For the ^5^1Ti and ^5^1Cr yields, there are some discrepancies between the present and reported ones. The yield corrected for the secondaries, in units of μb/equivalent quantum, were unfolded into cross sections per photon, in units of μb, as a function ol monochromatic photon energy with the LOUHI-82 code. The results for the ^5^1Ti and ^4^9Cr are in disagreement in both the magnitude and shape with the theoretical predictions based on DWIA and PWIA. A Monte Carlo calculation based on the PICA code by Gabriel and Alsmiller does reproduce the gross feature of the present results. |
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Chromium and titanium isotopes produced in photonuclear reactions of vanadium, revisited |
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| author2 |
Sakamoto, K. Yoshida, M. Kubota, Y. Fukasawa, T. Kunugise, A. Hamajima, Y. Shibata, S. Fujiwara, I. |
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Sakamoto, K. Yoshida, M. Kubota, Y. Fukasawa, T. Kunugise, A. Hamajima, Y. Shibata, S. Fujiwara, I. |
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