PANDORA Project for the study of photonuclear reactions below A= 60

A. Tamii; L. Pellegri; P. A. Söderström; D. Allard; S. Goriely; T. Inakura; E. Khan; E. Kido; M. Kimura; E. Litvinova; S. Nagataki; P. von Neumann-Cosel; N. Pietralla; N. Shimizu; N. Tsoneva; Y. Utsuno; S. Adachi; P. Adsley; A. Bahini; D. Balabanski; B. Baret; J. A.C. Bekker; S. D. Binda; E. Boicu; A. Bracco; I. Brandherm; M. Brezeanu; J. W. Brummer; F. Camera; F. C.L. Crespi; R. Dalal; L. M. Donaldson; Y. Fujikawa; T. Furuno; H. Haoning; R. Higuchi; Y. Honda; A. Gavrilescu; A. Inoue; J. Isaak; H. Jivan; P. Jones; S. Jongile; O. Just; T. Kawabata; T. Khumalo; J. Kiener; J. Kleemann; N. Kobayashi; Y. Koshio; A. Kuşoğlu; K. C.W. Li; K. L. Malatji; R. E. Molaeng; H. Motoki; M. Murata; A. A. Netshiya; R. Neveling; R. Niina; S. Okamoto; S. Ota; O. Papst; E. Parizot; T. Petruse; M. S. Reen; P. Ring; K. Sakanashi; E. Sideras-Haddad; S. Siem; M. Spall; T. Suda; T. Sudo; Y. Taniguchi; V. Tatischeff; H. Utsunomiya; H. Wang; V. Werner; H. Wibowo; M. Wiedeking; O. Wieland; Y. Xu; Z. H. Yang

doi:10.1140/epja/s10050-023-01081-w

PANDORA Project for the study of photonuclear reactions below A= 60

A. Tamii
, L. Pellegri
, P. A. Söderström
, D. Allard
, S. Goriely
, T. Inakura
, E. Khan
, E. Kido
, M. Kimura
, E. Litvinova
, S. Nagataki
, P. von Neumann-Cosel
, N. Pietralla
, N. Shimizu
, N. Tsoneva
, Y. Utsuno
, S. Adachi
, P. Adsley
, A. Bahini
, D. Balabanski

B. Baret, J. A.C. Bekker, S. D. Binda, E. Boicu, A. Bracco, I. Brandherm, M. Brezeanu, J. W. Brummer, F. Camera, F. C.L. Crespi, R. Dalal, L. M. Donaldson, Y. Fujikawa, T. Furuno, H. Haoning, R. Higuchi, Y. Honda, A. Gavrilescu, A. Inoue, J. Isaak, H. Jivan, P. Jones, S. Jongile, O. Just, T. Kawabata, T. Khumalo, J. Kiener, J. Kleemann, N. Kobayashi, Y. Koshio, A. Kuşoğlu, K. C.W. Li, K. L. Malatji, R. E. Molaeng, H. Motoki, M. Murata, A. A. Netshiya, R. Neveling, R. Niina, S. Okamoto, S. Ota, O. Papst, E. Parizot, T. Petruse, M. S. Reen, P. Ring, K. Sakanashi, E. Sideras-Haddad, S. Siem, M. Spall, T. Suda, T. Sudo, Y. Taniguchi, V. Tatischeff, H. Utsunomiya, H. Wang, V. Werner, H. Wibowo, M. Wiedeking, O. Wieland, Y. Xu, Z. H. Yang

Department of Physics

Osaka University
University of the Witwatersrand, Johannesburg
iThemba Laboratory for Accelerator Based Sciences
Horia Hulubei National Institute of Physics and Nuclear Engineering
Université Paris Diderot
Université Libre de Bruxelles
Tokyo Institute of Technology
University Paris-Sud
Riken
Hokkaido University
Western Michigan University
Technische Universität Darmstadt
Tsukuba University
Japan Atomic Energy Agency
Tohoku University
Texas A and M University
University of Bucharest
University of Milan
INFN Sezione di Milano
Guru Jambheshwar University of Science and Technology
Kyoto University
University Politehnica of Bucharest
GSI Helmholtz Center
Okayama University
Istanbul University
University of Oslo
Frere Hospital and Walter Sisulu University
Akal University
National Institute of Technology
Shanghai Advanced Research Institute, Chinese Academy of Sciences
Konan University
Shanghai Institute of Applied Physics, Chinese Academy of Sciences
University of Chinese Academy of Sciences
University of York
State Key Laboratory of Nuclear Physics and Technology

Research output: Contribution to journal › Article › peer-review

19 Scopus citations

Abstract

Photonuclear reactions of light nuclei below a mass of A= 60 are planned to be studied experimentally and theoretically with the PANDORA (Photo-Absorption of Nuclei and Decay Observation for Reactions in Astrophysics) project. Two experimental methods, virtual photon excitation by proton scattering and real photo absorption by a high-brilliance γ -ray beam produced by laser Compton scattering, will be applied to measure the photoabsorption cross sections and decay branching ratio of each decay channel as a function of the photon energy. Several nuclear models, e.g. anti-symmetrized molecular dynamics, mean-field and beyond-mean-field models, a large-scale shell model, and ab initio models, will be employed to predict the photonuclear reactions. The uncertainty in the model predictions will be evaluated based on the discrepancies between the model predictions and experimental data. The data and predictions will be implemented in the general reaction calculation code, TALYS. The results will be applied to the simulation of the photo-disintegration process of ultra-high-energy cosmic rays in inter-galactic propagation.

Original language	English
Article number	208
Journal	European Physical Journal A
Volume	59
Issue number	9
DOIs	https://doi.org/10.1140/epja/s10050-023-01081-w
State	Published - Sep 2023

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Tamii, A., Pellegri, L., Söderström, P. A., Allard, D., Goriely, S., Inakura, T., Khan, E., Kido, E., Kimura, M., Litvinova, E., Nagataki, S., Neumann-Cosel, P. V., Pietralla, N., Shimizu, N., Tsoneva, N., Utsuno, Y., Adachi, S., Adsley, P., Bahini, A., ... Yang, Z. H. (2023). PANDORA Project for the study of photonuclear reactions below A= 60. European Physical Journal A, 59(9), Article 208. https://doi.org/10.1140/epja/s10050-023-01081-w

@article{b2be14ce29ef42f2af800f24686ec77c,

title = "PANDORA Project for the study of photonuclear reactions below A= 60",

abstract = "Photonuclear reactions of light nuclei below a mass of A= 60 are planned to be studied experimentally and theoretically with the PANDORA (Photo-Absorption of Nuclei and Decay Observation for Reactions in Astrophysics) project. Two experimental methods, virtual photon excitation by proton scattering and real photo absorption by a high-brilliance γ -ray beam produced by laser Compton scattering, will be applied to measure the photoabsorption cross sections and decay branching ratio of each decay channel as a function of the photon energy. Several nuclear models, e.g. anti-symmetrized molecular dynamics, mean-field and beyond-mean-field models, a large-scale shell model, and ab initio models, will be employed to predict the photonuclear reactions. The uncertainty in the model predictions will be evaluated based on the discrepancies between the model predictions and experimental data. The data and predictions will be implemented in the general reaction calculation code, TALYS. The results will be applied to the simulation of the photo-disintegration process of ultra-high-energy cosmic rays in inter-galactic propagation.",

author = "A. Tamii and L. Pellegri and S{\"o}derstr{\"o}m, \{P. A.\} and D. Allard and S. Goriely and T. Inakura and E. Khan and E. Kido and M. Kimura and E. Litvinova and S. Nagataki and Neumann-Cosel, \{P. von\} and N. Pietralla and N. Shimizu and N. Tsoneva and Y. Utsuno and S. Adachi and P. Adsley and A. Bahini and D. Balabanski and B. Baret and Bekker, \{J. A.C.\} and Binda, \{S. D.\} and E. Boicu and A. Bracco and I. Brandherm and M. Brezeanu and Brummer, \{J. W.\} and F. Camera and Crespi, \{F. C.L.\} and R. Dalal and Donaldson, \{L. M.\} and Y. Fujikawa and T. Furuno and H. Haoning and R. Higuchi and Y. Honda and A. Gavrilescu and A. Inoue and J. Isaak and H. Jivan and P. Jones and S. Jongile and O. Just and T. Kawabata and T. Khumalo and J. Kiener and J. Kleemann and N. Kobayashi and Y. Koshio and A. Ku{\c s}oğlu and Li, \{K. C.W.\} and Malatji, \{K. L.\} and Molaeng, \{R. E.\} and H. Motoki and M. Murata and Netshiya, \{A. A.\} and R. Neveling and R. Niina and S. Okamoto and S. Ota and O. Papst and E. Parizot and T. Petruse and Reen, \{M. S.\} and P. Ring and K. Sakanashi and E. Sideras-Haddad and S. Siem and M. Spall and T. Suda and T. Sudo and Y. Taniguchi and V. Tatischeff and H. Utsunomiya and H. Wang and V. Werner and H. Wibowo and M. Wiedeking and O. Wieland and Y. Xu and Yang, \{Z. H.\}",

note = "Publisher Copyright: {\textcopyright} 2023, The Author(s).",

year = "2023",

month = sep,

doi = "10.1140/epja/s10050-023-01081-w",

language = "English",

volume = "59",

journal = "European Physical Journal A",

issn = "1434-6001",

publisher = "Springer",

number = "9",

}

Tamii, A, Pellegri, L, Söderström, PA, Allard, D, Goriely, S, Inakura, T, Khan, E, Kido, E, Kimura, M, Litvinova, E, Nagataki, S, Neumann-Cosel, PV, Pietralla, N, Shimizu, N, Tsoneva, N, Utsuno, Y, Adachi, S, Adsley, P, Bahini, A, Balabanski, D, Baret, B, Bekker, JAC, Binda, SD, Boicu, E, Bracco, A, Brandherm, I, Brezeanu, M, Brummer, JW, Camera, F, Crespi, FCL, Dalal, R, Donaldson, LM, Fujikawa, Y, Furuno, T, Haoning, H, Higuchi, R, Honda, Y, Gavrilescu, A, Inoue, A, Isaak, J, Jivan, H, Jones, P, Jongile, S, Just, O, Kawabata, T, Khumalo, T, Kiener, J, Kleemann, J, Kobayashi, N, Koshio, Y, Kuşoğlu, A, Li, KCW, Malatji, KL, Molaeng, RE, Motoki, H, Murata, M, Netshiya, AA, Neveling, R, Niina, R, Okamoto, S, Ota, S, Papst, O, Parizot, E, Petruse, T, Reen, MS, Ring, P, Sakanashi, K, Sideras-Haddad, E, Siem, S, Spall, M, Suda, T, Sudo, T, Taniguchi, Y, Tatischeff, V, Utsunomiya, H, Wang, H, Werner, V, Wibowo, H, Wiedeking, M, Wieland, O, Xu, Y & Yang, ZH 2023, 'PANDORA Project for the study of photonuclear reactions below A= 60', European Physical Journal A, vol. 59, no. 9, 208. https://doi.org/10.1140/epja/s10050-023-01081-w

TY - JOUR

T1 - PANDORA Project for the study of photonuclear reactions below A= 60

AU - Tamii, A.

AU - Pellegri, L.

AU - Söderström, P. A.

AU - Allard, D.

AU - Goriely, S.

AU - Inakura, T.

AU - Khan, E.

AU - Kido, E.

AU - Kimura, M.

AU - Litvinova, E.

AU - Nagataki, S.

AU - Neumann-Cosel, P. von

AU - Pietralla, N.

AU - Shimizu, N.

AU - Tsoneva, N.

AU - Utsuno, Y.

AU - Adachi, S.

AU - Adsley, P.

AU - Bahini, A.

AU - Balabanski, D.

AU - Baret, B.

AU - Bekker, J. A.C.

AU - Binda, S. D.

AU - Boicu, E.

AU - Bracco, A.

AU - Brandherm, I.

AU - Brezeanu, M.

AU - Brummer, J. W.

AU - Camera, F.

AU - Crespi, F. C.L.

AU - Dalal, R.

AU - Donaldson, L. M.

AU - Fujikawa, Y.

AU - Furuno, T.

AU - Haoning, H.

AU - Higuchi, R.

AU - Honda, Y.

AU - Gavrilescu, A.

AU - Inoue, A.

AU - Isaak, J.

AU - Jivan, H.

AU - Jones, P.

AU - Jongile, S.

AU - Just, O.

AU - Kawabata, T.

AU - Khumalo, T.

AU - Kiener, J.

AU - Kleemann, J.

AU - Kobayashi, N.

AU - Koshio, Y.

AU - Kuşoğlu, A.

AU - Li, K. C.W.

AU - Malatji, K. L.

AU - Molaeng, R. E.

AU - Motoki, H.

AU - Murata, M.

AU - Netshiya, A. A.

AU - Neveling, R.

AU - Niina, R.

AU - Okamoto, S.

AU - Ota, S.

AU - Papst, O.

AU - Parizot, E.

AU - Petruse, T.

AU - Reen, M. S.

AU - Ring, P.

AU - Sakanashi, K.

AU - Sideras-Haddad, E.

AU - Siem, S.

AU - Spall, M.

AU - Suda, T.

AU - Sudo, T.

AU - Taniguchi, Y.

AU - Tatischeff, V.

AU - Utsunomiya, H.

AU - Wang, H.

AU - Werner, V.

AU - Wibowo, H.

AU - Wiedeking, M.

AU - Wieland, O.

AU - Xu, Y.

AU - Yang, Z. H.

PY - 2023/9

Y1 - 2023/9

N2 - Photonuclear reactions of light nuclei below a mass of A= 60 are planned to be studied experimentally and theoretically with the PANDORA (Photo-Absorption of Nuclei and Decay Observation for Reactions in Astrophysics) project. Two experimental methods, virtual photon excitation by proton scattering and real photo absorption by a high-brilliance γ -ray beam produced by laser Compton scattering, will be applied to measure the photoabsorption cross sections and decay branching ratio of each decay channel as a function of the photon energy. Several nuclear models, e.g. anti-symmetrized molecular dynamics, mean-field and beyond-mean-field models, a large-scale shell model, and ab initio models, will be employed to predict the photonuclear reactions. The uncertainty in the model predictions will be evaluated based on the discrepancies between the model predictions and experimental data. The data and predictions will be implemented in the general reaction calculation code, TALYS. The results will be applied to the simulation of the photo-disintegration process of ultra-high-energy cosmic rays in inter-galactic propagation.

AB - Photonuclear reactions of light nuclei below a mass of A= 60 are planned to be studied experimentally and theoretically with the PANDORA (Photo-Absorption of Nuclei and Decay Observation for Reactions in Astrophysics) project. Two experimental methods, virtual photon excitation by proton scattering and real photo absorption by a high-brilliance γ -ray beam produced by laser Compton scattering, will be applied to measure the photoabsorption cross sections and decay branching ratio of each decay channel as a function of the photon energy. Several nuclear models, e.g. anti-symmetrized molecular dynamics, mean-field and beyond-mean-field models, a large-scale shell model, and ab initio models, will be employed to predict the photonuclear reactions. The uncertainty in the model predictions will be evaluated based on the discrepancies between the model predictions and experimental data. The data and predictions will be implemented in the general reaction calculation code, TALYS. The results will be applied to the simulation of the photo-disintegration process of ultra-high-energy cosmic rays in inter-galactic propagation.

UR - https://www.scopus.com/pages/publications/85170657047

U2 - 10.1140/epja/s10050-023-01081-w

DO - 10.1140/epja/s10050-023-01081-w

M3 - Article

AN - SCOPUS:85170657047

SN - 1434-6001

VL - 59

JO - European Physical Journal A

JF - European Physical Journal A

IS - 9

M1 - 208

ER -

PANDORA Project for the study of photonuclear reactions below A= 60

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