Nuclear physics midterm plan at Legnaro National Laboratories (LNL)

M. Ballan; S. Bottoni; M. Caamaño; A. Caciolli; M. Campostrini; M. Cicerchia; F. C.L. Crespi; S. Cristallo; D. Dell’Aquila; R. Depalo; E. Fioretto; F. Galtarossa; L. R. Gasques; A. Gottardo; F. Gramegna; F. Gulminelli; T. Kurtukian-Nieto; M. La Cognata; S. M. Lenzi; T. Marchi; K. Mazurek; D. Mengoni; L. Mou; R. Nania; G. Pupillo; J. J. Valiente-Dobón; I. Zanon; L. Acosta; M. A.G. Alvarez; A. Andrighetto; A. Arazi; A. Arzenton; M. Assié; M. Bagatin; F. Barbaro; C. Barbieri; S. Barlini; L. Basiricò; G. Battistoni; D. Beaumel; M. A. Bentley; G. Benzoni; S. Bertoldo; C. Bertulani; A. Bonasera; A. Camaiani; L. Canton; V. Capirossi; M. P. Carante; C. Carraro; S. M. Carturan; G. Casini; F. Cavanna; L. Centofante; E. R. Chávez; A. Chbihi; M. Ciemała; S. Cisternino; A. Colombi; M. Colucci; A. Compagnucci; S. Corradetti; L. Corradi; G. D’Agata; G. de Angelis; L. De Dominicis; D. De Salvador; E. DeFilippo; M. Del Fabbro; A. Di Nitto; S. Ditalia Tchernij; A. Donzella; T. Duguet; J. Esposito; F. Favela; J. P. Fernández-García; F. Flavigny; A. Fontana; B. Fornal; J. Forneris; B. Fraboni; J. Frankland; E. Gamba; E. Geraci; S. Gerardin; S. A. Giuliani; B. Gnoffo; F. Groppi; D. Gruyer; F. Haddad; J. Isaak; M. Kmiecik; A. Koning; L. Lamia; N. Le Neindre; S. Leoni; A. Lépine-Szily; G. Lilli; I. Lombardo; M. Loriggiola; L. Loriggiola; M. Lunardon; G. Maggioni; A. Maj; S. Manenti; M. Manzolaro; L. E. Marcucci; D. J. Marín-Lámbarri; E. Mariotti; G. Martin Hernandez; C. Massimi; P. Mastinu; M. Mazzocco; T. Mijatović; T. Mishenina; K. Mizuyama; A. Monetti; G. Montagnoli; L. Morselli; L. Moschini; E. Musacchio Gonzalez; A. Nannini; Y. F. Niu; S. Ota; A. Paccagnella; S. Palmerini; L. Pellegri; A. Perego; S. Piantelli; D. Piatti; F. Picollo; M. Pignatari; F. Pinna; S. Pirrone; R. G. Pizzone; M. Polettini; G. Politi; L. Popescu; G. Prete; A. Quaranta; R. Raabe; J. P. Ramos; W. Raniero; G. G. Rapisarda; F. Recchia; V. Rigato; X. Roca Maza; M. Rocchini; T. Rodriguez; C. Roncolato; D. Rudolph; P. Russotto; M. Sánchez-Benítez; D. Savran; D. Scarpa; M. Scheck; K. Sekizawa; M. L. Sergi; F. Sgarbossa; L. Silvestrin; O. Singh Khwairakpam; J. Skowronski; V. Somà; R. Spartà; M. Spieker; A. M. Stefanini; H. Steiger; L. Stevanato; M. R. Stock; E. Vardaci; D. Verney; D. Vescovi; E. Vittone; V. Werner; C. Wheldon; O. Wieland; K. Wimmer; J. Wyss; L. Zago; A. Zenoni

doi:10.1140/epjp/s13360-023-04249-x

Nuclear physics midterm plan at Legnaro National Laboratories (LNL)

M. Ballan, S. Bottoni, M. Caamaño, A. Caciolli, M. Campostrini, M. Cicerchia, F. C.L. Crespi, S. Cristallo, D. Dell’Aquila, R. Depalo, E. Fioretto, F. Galtarossa, L. R. Gasques, A. Gottardo, F. Gramegna, F. Gulminelli, T. Kurtukian-Nieto, M. La Cognata, S. M. Lenzi, T. MarchiK. Mazurek, D. Mengoni^*, L. Mou, R. Nania, G. Pupillo, J. J. Valiente-Dobón^*, I. Zanon, L. Acosta, M. A.G. Alvarez, A. Andrighetto, A. Arazi, A. Arzenton, M. Assié, M. Bagatin, F. Barbaro, C. Barbieri, S. Barlini, L. Basiricò, G. Battistoni, D. Beaumel, M. A. Bentley, G. Benzoni, S. Bertoldo, C. Bertulani, A. Bonasera, A. Camaiani, L. Canton, V. Capirossi, M. P. Carante, C. Carraro, S. M. Carturan, G. Casini, F. Cavanna, L. Centofante, E. R. Chávez, A. Chbihi, M. Ciemała, S. Cisternino, A. Colombi, M. Colucci, A. Compagnucci, S. Corradetti, L. Corradi, G. D’Agata, G. de Angelis, L. De Dominicis, D. De Salvador, E. DeFilippo, M. Del Fabbro, A. Di Nitto, S. Ditalia Tchernij, A. Donzella, T. Duguet, J. Esposito, F. Favela, J. P. Fernández-García, F. Flavigny, A. Fontana, B. Fornal, J. Forneris, B. Fraboni, J. Frankland, E. Gamba, E. Geraci, S. Gerardin, S. A. Giuliani, B. Gnoffo, F. Groppi, D. Gruyer, F. Haddad, J. Isaak, M. Kmiecik, A. Koning, L. Lamia, N. Le Neindre, S. Leoni, A. Lépine-Szily, G. Lilli, I. Lombardo, M. Loriggiola, L. Loriggiola, M. Lunardon, G. Maggioni, A. Maj, S. Manenti, M. Manzolaro, L. E. Marcucci, D. J. Marín-Lámbarri, E. Mariotti, G. Martin Hernandez, C. Massimi, P. Mastinu, M. Mazzocco, T. Mijatović, T. Mishenina, K. Mizuyama, A. Monetti, G. Montagnoli, L. Morselli, L. Moschini, E. Musacchio Gonzalez, A. Nannini, Y. F. Niu, S. Ota, A. Paccagnella, S. Palmerini, L. Pellegri, A. Perego, S. Piantelli, D. Piatti, F. Picollo, M. Pignatari, F. Pinna, S. Pirrone, R. G. Pizzone, M. Polettini, G. Politi, L. Popescu, G. Prete, A. Quaranta, R. Raabe, J. P. Ramos, W. Raniero, G. G. Rapisarda, F. Recchia, V. Rigato, X. Roca Maza, M. Rocchini, T. Rodriguez, C. Roncolato, D. Rudolph, P. Russotto, M. Sánchez-Benítez, D. Savran, D. Scarpa, M. Scheck, K. Sekizawa, M. L. Sergi, F. Sgarbossa, L. Silvestrin, O. Singh Khwairakpam, J. Skowronski, V. Somà, R. Spartà, M. Spieker, A. M. Stefanini, H. Steiger, L. Stevanato, M. R. Stock, E. Vardaci, D. Verney, D. Vescovi, E. Vittone, V. Werner, C. Wheldon, O. Wieland, K. Wimmer, J. Wyss, L. Zago, A. Zenoni

^*Corresponding author for this work

Physics

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

Abstract

The next years will see the completion of the radioactive ion beam facility SPES (Selective Production of Exotic Species) and the upgrade of the accelerators complex at Istituto Nazionale di Fisica Nucleare – Legnaro National Laboratories (LNL) opening up new possibilities in the fields of nuclear structure, nuclear dynamics, nuclear astrophysics, and applications. The nuclear physics community has organised a workshop to discuss the new physics opportunities that will be possible in the near future by employing state-of-the-art detection systems. A detailed discussion of the outcome from the workshop is presented in this report.

Original language	English
Article number	709
Journal	European Physical Journal Plus
Volume	138
Issue number	8
DOIs	https://doi.org/10.1140/epjp/s13360-023-04249-x
Publication status	Published - 14 Aug 2023

Bibliographical note

Funding Information:
Open access funding provided by Università degli Studi di Padova within the CRUI-CARE Agreement.

Funding Information:
The NEPIR-0 is almost completely funded by the Italian Ministry for University Research (MUR), within the Italian SPARE (Space Radiation Shielding) project that deals with health risks due to cosmic radiation. In this phase the neutron source is a relatively simple, thick, low power (100 W) beryllium target located inside the conduit between the cyclotron hall and experimental hall of the SPES building []. The 3 m thick wall of the cyclotron cave provides shielding and the conduit acts as a collimator for the neutron beam directed to the neutron’s experimental area. The expected neutron beam has a continuum spectrum with a different cut-off according to different proton energies. In this phase, a low proton current will be used ( 1 A) to reduce the radiation protection problems. The phase-0 facility will be open to academic and industrial users, to test microelectronic components and devices, for neutron detector characterization, and neutron shielding materials for space missions, in partnership with ASI.

Publisher Copyright:
© 2023, The Author(s).

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10.1140/epjp/s13360-023-04249-xLicence: CC BY

Nuclear physics midterm plan at Legnaro National Laboratories (LNL)Final published version, 5.54 MBLicence: CC BY

Cite this

Ballan, M., Bottoni, S., Caamaño, M., Caciolli, A., Campostrini, M., Cicerchia, M., Crespi, F. C. L., Cristallo, S., Dell’Aquila, D., Depalo, R., Fioretto, E., Galtarossa, F., Gasques, L. R., Gottardo, A., Gramegna, F., Gulminelli, F., Kurtukian-Nieto, T., La Cognata, M., Lenzi, S. M., ... Zenoni, A. (2023). Nuclear physics midterm plan at Legnaro National Laboratories (LNL). European Physical Journal Plus, 138(8), Article 709. https://doi.org/10.1140/epjp/s13360-023-04249-x

@article{a6722f5ba8fe4f2f8f95709ffa5c85e4,

title = "Nuclear physics midterm plan at Legnaro National Laboratories (LNL)",

abstract = "The next years will see the completion of the radioactive ion beam facility SPES (Selective Production of Exotic Species) and the upgrade of the accelerators complex at Istituto Nazionale di Fisica Nucleare – Legnaro National Laboratories (LNL) opening up new possibilities in the fields of nuclear structure, nuclear dynamics, nuclear astrophysics, and applications. The nuclear physics community has organised a workshop to discuss the new physics opportunities that will be possible in the near future by employing state-of-the-art detection systems. A detailed discussion of the outcome from the workshop is presented in this report.",

author = "M. Ballan and S. Bottoni and M. Caama{\~n}o and A. Caciolli and M. Campostrini and M. Cicerchia and Crespi, {F. C.L.} and S. Cristallo and D. Dell{\textquoteright}Aquila and R. Depalo and E. Fioretto and F. Galtarossa and Gasques, {L. R.} and A. Gottardo and F. Gramegna and F. Gulminelli and T. Kurtukian-Nieto and {La Cognata}, M. and Lenzi, {S. M.} and T. Marchi and K. Mazurek and D. Mengoni and L. Mou and R. Nania and G. Pupillo and Valiente-Dob{\'o}n, {J. J.} and I. Zanon and L. Acosta and Alvarez, {M. A.G.} and A. Andrighetto and A. Arazi and A. Arzenton and M. Assi{\'e} and M. Bagatin and F. Barbaro and C. Barbieri and S. Barlini and L. Basiric{\`o} and G. Battistoni and D. Beaumel and Bentley, {M. A.} and G. Benzoni and S. Bertoldo and C. Bertulani and A. Bonasera and A. Camaiani and L. Canton and V. Capirossi and Carante, {M. P.} and C. Carraro and Carturan, {S. M.} and G. Casini and F. Cavanna and L. Centofante and Ch{\'a}vez, {E. R.} and A. Chbihi and M. Ciema{\l}a and S. Cisternino and A. Colombi and M. Colucci and A. Compagnucci and S. Corradetti and L. Corradi and G. D{\textquoteright}Agata and {de Angelis}, G. and {De Dominicis}, L. and {De Salvador}, D. and E. DeFilippo and {Del Fabbro}, M. and {Di Nitto}, A. and {Ditalia Tchernij}, S. and A. Donzella and T. Duguet and J. Esposito and F. Favela and Fern{\'a}ndez-Garc{\'i}a, {J. P.} and F. Flavigny and A. Fontana and B. Fornal and J. Forneris and B. Fraboni and J. Frankland and E. Gamba and E. Geraci and S. Gerardin and Giuliani, {S. A.} and B. Gnoffo and F. Groppi and D. Gruyer and F. Haddad and J. Isaak and M. Kmiecik and A. Koning and L. Lamia and {Le Neindre}, N. and S. Leoni and A. L{\'e}pine-Szily and G. Lilli and I. Lombardo and M. Loriggiola and L. Loriggiola and M. Lunardon and G. Maggioni and A. Maj and S. Manenti and M. Manzolaro and Marcucci, {L. E.} and Mar{\'i}n-L{\'a}mbarri, {D. J.} and E. Mariotti and {Martin Hernandez}, G. and C. Massimi and P. Mastinu and M. Mazzocco and T. Mijatovi{\'c} and T. Mishenina and K. Mizuyama and A. Monetti and G. Montagnoli and L. Morselli and L. Moschini and {Musacchio Gonzalez}, E. and A. Nannini and Niu, {Y. F.} and S. Ota and A. Paccagnella and S. Palmerini and L. Pellegri and A. Perego and S. Piantelli and D. Piatti and F. Picollo and M. Pignatari and F. Pinna and S. Pirrone and Pizzone, {R. G.} and M. Polettini and G. Politi and L. Popescu and G. Prete and A. Quaranta and R. Raabe and Ramos, {J. P.} and W. Raniero and Rapisarda, {G. G.} and F. Recchia and V. Rigato and {Roca Maza}, X. and M. Rocchini and T. Rodriguez and C. Roncolato and D. Rudolph and P. Russotto and M. S{\'a}nchez-Ben{\'i}tez and D. Savran and D. Scarpa and M. Scheck and K. Sekizawa and Sergi, {M. L.} and F. Sgarbossa and L. Silvestrin and {Singh Khwairakpam}, O. and J. Skowronski and V. Som{\`a} and R. Spart{\`a} and M. Spieker and Stefanini, {A. M.} and H. Steiger and L. Stevanato and Stock, {M. R.} and E. Vardaci and D. Verney and D. Vescovi and E. Vittone and V. Werner and C. Wheldon and O. Wieland and K. Wimmer and J. Wyss and L. Zago and A. Zenoni",

note = "Funding Information: Open access funding provided by Universit{\`a} degli Studi di Padova within the CRUI-CARE Agreement. Funding Information: The NEPIR-0 is almost completely funded by the Italian Ministry for University Research (MUR), within the Italian SPARE (Space Radiation Shielding) project that deals with health risks due to cosmic radiation. In this phase the neutron source is a relatively simple, thick, low power (100 W) beryllium target located inside the conduit between the cyclotron hall and experimental hall of the SPES building []. The 3 m thick wall of the cyclotron cave provides shielding and the conduit acts as a collimator for the neutron beam directed to the neutron{\textquoteright}s experimental area. The expected neutron beam has a continuum spectrum with a different cut-off according to different proton energies. In this phase, a low proton current will be used ( 1 A) to reduce the radiation protection problems. The phase-0 facility will be open to academic and industrial users, to test microelectronic components and devices, for neutron detector characterization, and neutron shielding materials for space missions, in partnership with ASI. Publisher Copyright: {\textcopyright} 2023, The Author(s).",

year = "2023",

month = aug,

day = "14",

doi = "10.1140/epjp/s13360-023-04249-x",

language = "English",

volume = "138",

journal = "European Physical Journal Plus",

issn = "2190-5444",

publisher = "Springer",

number = "8",

}

Ballan, M, Bottoni, S, Caamaño, M, Caciolli, A, Campostrini, M, Cicerchia, M, Crespi, FCL, Cristallo, S, Dell’Aquila, D, Depalo, R, Fioretto, E, Galtarossa, F, Gasques, LR, Gottardo, A, Gramegna, F, Gulminelli, F, Kurtukian-Nieto, T, La Cognata, M, Lenzi, SM, Marchi, T, Mazurek, K, Mengoni, D, Mou, L, Nania, R, Pupillo, G, Valiente-Dobón, JJ, Zanon, I, Acosta, L, Alvarez, MAG, Andrighetto, A, Arazi, A, Arzenton, A, Assié, M, Bagatin, M, Barbaro, F, Barbieri, C, Barlini, S, Basiricò, L, Battistoni, G, Beaumel, D, Bentley, MA, Benzoni, G, Bertoldo, S, Bertulani, C, Bonasera, A, Camaiani, A, Canton, L, Capirossi, V, Carante, MP, Carraro, C, Carturan, SM, Casini, G, Cavanna, F, Centofante, L, Chávez, ER, Chbihi, A, Ciemała, M, Cisternino, S, Colombi, A, Colucci, M, Compagnucci, A, Corradetti, S, Corradi, L, D’Agata, G, de Angelis, G, De Dominicis, L, De Salvador, D, DeFilippo, E, Del Fabbro, M, Di Nitto, A, Ditalia Tchernij, S, Donzella, A, Duguet, T, Esposito, J, Favela, F, Fernández-García, JP, Flavigny, F, Fontana, A, Fornal, B, Forneris, J, Fraboni, B, Frankland, J, Gamba, E, Geraci, E, Gerardin, S, Giuliani, SA, Gnoffo, B, Groppi, F, Gruyer, D, Haddad, F, Isaak, J, Kmiecik, M, Koning, A, Lamia, L, Le Neindre, N, Leoni, S, Lépine-Szily, A, Lilli, G, Lombardo, I, Loriggiola, M, Loriggiola, L, Lunardon, M, Maggioni, G, Maj, A, Manenti, S, Manzolaro, M, Marcucci, LE, Marín-Lámbarri, DJ, Mariotti, E, Martin Hernandez, G, Massimi, C, Mastinu, P, Mazzocco, M, Mijatović, T, Mishenina, T, Mizuyama, K, Monetti, A, Montagnoli, G, Morselli, L, Moschini, L, Musacchio Gonzalez, E, Nannini, A, Niu, YF, Ota, S, Paccagnella, A, Palmerini, S, Pellegri, L, Perego, A, Piantelli, S, Piatti, D, Picollo, F, Pignatari, M, Pinna, F, Pirrone, S, Pizzone, RG, Polettini, M, Politi, G, Popescu, L, Prete, G, Quaranta, A, Raabe, R, Ramos, JP, Raniero, W, Rapisarda, GG, Recchia, F, Rigato, V, Roca Maza, X, Rocchini, M, Rodriguez, T, Roncolato, C, Rudolph, D, Russotto, P, Sánchez-Benítez, M, Savran, D, Scarpa, D, Scheck, M, Sekizawa, K, Sergi, ML, Sgarbossa, F, Silvestrin, L, Singh Khwairakpam, O, Skowronski, J, Somà, V, Spartà, R, Spieker, M, Stefanini, AM, Steiger, H, Stevanato, L, Stock, MR, Vardaci, E, Verney, D, Vescovi, D, Vittone, E, Werner, V, Wheldon, C, Wieland, O, Wimmer, K, Wyss, J, Zago, L & Zenoni, A 2023, 'Nuclear physics midterm plan at Legnaro National Laboratories (LNL)', European Physical Journal Plus, vol. 138, no. 8, 709. https://doi.org/10.1140/epjp/s13360-023-04249-x

TY - JOUR

T1 - Nuclear physics midterm plan at Legnaro National Laboratories (LNL)

AU - Ballan, M.

AU - Bottoni, S.

AU - Caamaño, M.

AU - Caciolli, A.

AU - Campostrini, M.

AU - Cicerchia, M.

AU - Crespi, F. C.L.

AU - Cristallo, S.

AU - Dell’Aquila, D.

AU - Depalo, R.

AU - Fioretto, E.

AU - Galtarossa, F.

AU - Gasques, L. R.

AU - Gottardo, A.

AU - Gramegna, F.

AU - Gulminelli, F.

AU - Kurtukian-Nieto, T.

AU - La Cognata, M.

AU - Lenzi, S. M.

AU - Marchi, T.

AU - Mazurek, K.

AU - Mengoni, D.

AU - Mou, L.

AU - Nania, R.

AU - Pupillo, G.

AU - Valiente-Dobón, J. J.

AU - Zanon, I.

AU - Acosta, L.

AU - Alvarez, M. A.G.

AU - Andrighetto, A.

AU - Arazi, A.

AU - Arzenton, A.

AU - Assié, M.

AU - Bagatin, M.

AU - Barbaro, F.

AU - Barbieri, C.

AU - Barlini, S.

AU - Basiricò, L.

AU - Battistoni, G.

AU - Beaumel, D.

AU - Bentley, M. A.

AU - Benzoni, G.

AU - Bertoldo, S.

AU - Bertulani, C.

AU - Bonasera, A.

AU - Camaiani, A.

AU - Canton, L.

AU - Capirossi, V.

AU - Carante, M. P.

AU - Carraro, C.

AU - Carturan, S. M.

AU - Casini, G.

AU - Cavanna, F.

AU - Centofante, L.

AU - Chávez, E. R.

AU - Chbihi, A.

AU - Ciemała, M.

AU - Cisternino, S.

AU - Colombi, A.

AU - Colucci, M.

AU - Compagnucci, A.

AU - Corradetti, S.

AU - Corradi, L.

AU - D’Agata, G.

AU - de Angelis, G.

AU - De Dominicis, L.

AU - De Salvador, D.

AU - DeFilippo, E.

AU - Del Fabbro, M.

AU - Di Nitto, A.

AU - Ditalia Tchernij, S.

AU - Donzella, A.

AU - Duguet, T.

AU - Esposito, J.

AU - Favela, F.

AU - Fernández-García, J. P.

AU - Flavigny, F.

AU - Fontana, A.

AU - Fornal, B.

AU - Forneris, J.

AU - Fraboni, B.

AU - Frankland, J.

AU - Gamba, E.

AU - Geraci, E.

AU - Gerardin, S.

AU - Giuliani, S. A.

AU - Gnoffo, B.

AU - Groppi, F.

AU - Gruyer, D.

AU - Haddad, F.

AU - Isaak, J.

AU - Kmiecik, M.

AU - Koning, A.

AU - Lamia, L.

AU - Le Neindre, N.

AU - Leoni, S.

AU - Lépine-Szily, A.

AU - Lilli, G.

AU - Lombardo, I.

AU - Loriggiola, M.

AU - Loriggiola, L.

AU - Lunardon, M.

AU - Maggioni, G.

AU - Maj, A.

AU - Manenti, S.

AU - Manzolaro, M.

AU - Marcucci, L. E.

AU - Marín-Lámbarri, D. J.

AU - Mariotti, E.

AU - Martin Hernandez, G.

AU - Massimi, C.

AU - Mastinu, P.

AU - Mazzocco, M.

AU - Mijatović, T.

AU - Mishenina, T.

AU - Mizuyama, K.

AU - Monetti, A.

AU - Montagnoli, G.

AU - Morselli, L.

AU - Moschini, L.

AU - Musacchio Gonzalez, E.

AU - Nannini, A.

AU - Niu, Y. F.

AU - Ota, S.

AU - Paccagnella, A.

AU - Palmerini, S.

AU - Pellegri, L.

AU - Perego, A.

AU - Piantelli, S.

AU - Piatti, D.

AU - Picollo, F.

AU - Pignatari, M.

AU - Pinna, F.

AU - Pirrone, S.

AU - Pizzone, R. G.

AU - Polettini, M.

AU - Politi, G.

AU - Popescu, L.

AU - Prete, G.

AU - Quaranta, A.

AU - Raabe, R.

AU - Ramos, J. P.

AU - Raniero, W.

AU - Rapisarda, G. G.

AU - Recchia, F.

AU - Rigato, V.

AU - Roca Maza, X.

AU - Rocchini, M.

AU - Rodriguez, T.

AU - Roncolato, C.

AU - Rudolph, D.

AU - Russotto, P.

AU - Sánchez-Benítez, M.

AU - Savran, D.

AU - Scarpa, D.

AU - Scheck, M.

AU - Sekizawa, K.

AU - Sergi, M. L.

AU - Sgarbossa, F.

AU - Silvestrin, L.

AU - Singh Khwairakpam, O.

AU - Skowronski, J.

AU - Somà, V.

AU - Spartà, R.

AU - Spieker, M.

AU - Stefanini, A. M.

AU - Steiger, H.

AU - Stevanato, L.

AU - Stock, M. R.

AU - Vardaci, E.

AU - Verney, D.

AU - Vescovi, D.

AU - Vittone, E.

AU - Werner, V.

AU - Wheldon, C.

AU - Wieland, O.

AU - Wimmer, K.

AU - Wyss, J.

AU - Zago, L.

AU - Zenoni, A.

N1 - Funding Information: Open access funding provided by Università degli Studi di Padova within the CRUI-CARE Agreement. Funding Information: The NEPIR-0 is almost completely funded by the Italian Ministry for University Research (MUR), within the Italian SPARE (Space Radiation Shielding) project that deals with health risks due to cosmic radiation. In this phase the neutron source is a relatively simple, thick, low power (100 W) beryllium target located inside the conduit between the cyclotron hall and experimental hall of the SPES building []. The 3 m thick wall of the cyclotron cave provides shielding and the conduit acts as a collimator for the neutron beam directed to the neutron’s experimental area. The expected neutron beam has a continuum spectrum with a different cut-off according to different proton energies. In this phase, a low proton current will be used ( 1 A) to reduce the radiation protection problems. The phase-0 facility will be open to academic and industrial users, to test microelectronic components and devices, for neutron detector characterization, and neutron shielding materials for space missions, in partnership with ASI. Publisher Copyright: © 2023, The Author(s).

PY - 2023/8/14

Y1 - 2023/8/14

N2 - The next years will see the completion of the radioactive ion beam facility SPES (Selective Production of Exotic Species) and the upgrade of the accelerators complex at Istituto Nazionale di Fisica Nucleare – Legnaro National Laboratories (LNL) opening up new possibilities in the fields of nuclear structure, nuclear dynamics, nuclear astrophysics, and applications. The nuclear physics community has organised a workshop to discuss the new physics opportunities that will be possible in the near future by employing state-of-the-art detection systems. A detailed discussion of the outcome from the workshop is presented in this report.

AB - The next years will see the completion of the radioactive ion beam facility SPES (Selective Production of Exotic Species) and the upgrade of the accelerators complex at Istituto Nazionale di Fisica Nucleare – Legnaro National Laboratories (LNL) opening up new possibilities in the fields of nuclear structure, nuclear dynamics, nuclear astrophysics, and applications. The nuclear physics community has organised a workshop to discuss the new physics opportunities that will be possible in the near future by employing state-of-the-art detection systems. A detailed discussion of the outcome from the workshop is presented in this report.

UR - http://www.scopus.com/inward/record.url?scp=85168321420&partnerID=8YFLogxK

U2 - 10.1140/epjp/s13360-023-04249-x

DO - 10.1140/epjp/s13360-023-04249-x

M3 - Article

AN - SCOPUS:85168321420

SN - 2190-5444

VL - 138

JO - European Physical Journal Plus

JF - European Physical Journal Plus

IS - 8

M1 - 709

ER -

Nuclear physics midterm plan at Legnaro National Laboratories (LNL)

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