002916248 001__ 2916248
002916248 003__ SzGeCERN
002916248 005__ 20241105215206.0
002916248 0247_ $$2DOI$$9EDP Sciences$$a10.1051/epjconf/202328401018
002916248 0248_ $$aoai:cds.cern.ch:2916248$$pcerncds:FULLTEXT$$pcerncds:CERN:FULLTEXT$$pcerncds:CERN
002916248 035__ $$9NSR$$a2023DOZZ
002916248 035__ $$9https://inspirehep.net/api/oai2d$$aoai:inspirehep.net:2758587$$d2024-11-04T16:02:10Z$$h2024-11-05T05:21:33Z$$mmarcxml
002916248 035__ $$9Inspire$$a2758587
002916248 041__ $$aeng
002916248 100__ $$aDomingo-Pardo, C
002916248 245__ $$9EDP Sciences$$aCompton imaging for enhanced sensitivity (n,γ) cross section TOF experiments: Status and prospects
002916248 260__ $$c2023
002916248 300__ $$a5 p
002916248 520__ $$9EDP Sciences$$aRadiative neutron-capture cross sections are of pivotal importance in many fields such as nucle-osynthesis studies or innovative reactor technologies. A large number of isotopes have been measured with high accuracy, but there are still a large number of relevant isotopes whose cross sections could not be experimentally determined yet, at least with sufficient accuracy and completeness, owing to limitations in detection techniques, sample production methods or in the facilities themselves.In the context of the HYMNS (High-sensitivitY Measurements of key stellar Nucleo-Synthesis reactions) project over the last six years we have developed a novel detection technique aimed at background suppression in radiative neutron-capture time-of-flight measurements. This new technique utilizes a complex detection set-up based on position-sensitive radiation-detectors deployed in a Compton-camera array configuration. The latter enables to implement gamma-ray imaging techniques, which help to disentangle true capture events arising from the sample under study and contaminant background events from the surroundings. A summary on the main developments is given in this contribution together with an update on recent experiments at CERN n_TOF and an outlook on future steps.
002916248 540__ $$aCC-BY-4.0$$bEDP Sciences$$uhttps://creativecommons.org/licenses/by/4.0/
002916248 542__ $$3publication$$dThe authors$$g2023
002916248 65017 $$2SzGeCERN$$aNuclear Physics - Experiment
002916248 690C_ $$aARTICLE
002916248 690C_ $$aCERN
002916248 693__ $$aCERN PS$$enTOF
002916248 700__ $$aBabiano-Suarez, V
002916248 700__ $$aBalibrea-Correa, J
002916248 700__ $$aCaballero, L
002916248 700__ $$aLadarescu, I
002916248 700__ $$aLerendegui-Marco, J
002916248 700__ $$aTarifeño-Saldivia, A
002916248 700__ $$aAberle, O$$uCERN
002916248 700__ $$aAlcayne, V
002916248 700__ $$aAltieri, S$$vDepartment of Physics, University of Pavia, Italy
002916248 700__ $$aAmaducci, S
002916248 700__ $$aAndrzejewski, J
002916248 700__ $$aBacak, M$$uCERN
002916248 700__ $$aBeltrami, C
002916248 700__ $$aBennett, S
002916248 700__ $$aBernardes, A P$$uCERN
002916248 700__ $$aBerthoumieux, E
002916248 700__ $$aBeyer, R
002916248 700__ $$aBoromiza, M
002916248 700__ $$aBosnar, D
002916248 700__ $$aCaamaño, M
002916248 700__ $$aCalviño, F
002916248 700__ $$aCalviani, M$$uCERN
002916248 700__ $$aCano-Ott, D
002916248 700__ $$aCasanovas, A
002916248 700__ $$aCerutti, F$$uCERN
002916248 700__ $$aCescutti, G$$vDepartment of Physics, University of Trieste, Italy
002916248 700__ $$aChiaveri, E$$uCERN$$uManchester U.$$vUniversity of Manchester, United Kingdom
002916248 700__ $$aColombetti, P$$vDepartment of Physics, University of Torino, Italy
002916248 700__ $$aColonna, N
002916248 700__ $$aCamprini, P Console$$vAgenzia nazionale per le nuove tecnologie (ENEA), Italy
002916248 700__ $$aCortés, G
002916248 700__ $$aCortés-Giraldo, M A
002916248 700__ $$aCosentino, L
002916248 700__ $$aCristallo, S$$vIstituto Nazionale di Astrofisica - Osservatorio Astronomico di Teramo, Italy
002916248 700__ $$aDellmann, S
002916248 700__ $$aCastro, M Di$$uCERN
002916248 700__ $$aMaria, S Di
002916248 700__ $$aDiakaki, M
002916248 700__ $$aDietz, M
002916248 700__ $$aDressler, R
002916248 700__ $$aDupont, E
002916248 700__ $$aDurán, I
002916248 700__ $$aEleme, Z
002916248 700__ $$aFargier, S$$uCERN
002916248 700__ $$aFernández, B
002916248 700__ $$aFernández-Domínguez, B
002916248 700__ $$aFinocchiaro, P
002916248 700__ $$aFiore, S$$vIstituto Nazionale di Fisica Nucleare, Sezione di Roma1, Roma, Italy
002916248 700__ $$aGarcía-Infantes, F
002916248 700__ $$aGawlik-Ramie˛ga, A
002916248 700__ $$aGervino, G$$vDepartment of Physics, University of Torino, Italy
002916248 700__ $$aGilardoni, S$$uCERN
002916248 700__ $$aGonzález-Romero, E$$uCERN$$uMadrid, CIEMAT$$vCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Spain
002916248 700__ $$aGuerrero, C
002916248 700__ $$aGunsing, F
002916248 700__ $$aGustavino, C
002916248 700__ $$aHeyse, J
002916248 700__ $$aHillman, W
002916248 700__ $$aJenkins, D G
002916248 700__ $$aJericha, E
002916248 700__ $$aJunghans, A
002916248 700__ $$aKadi, Y$$uCERN
002916248 700__ $$aKaperoni, K
002916248 700__ $$aKaur, G
002916248 700__ $$aKimura, A
002916248 700__ $$aKnapová, I
002916248 700__ $$aKokkoris, M
002916248 700__ $$aKöster, U
002916248 700__ $$aKrtička, M
002916248 700__ $$aKyritsis, N
002916248 700__ $$aLederer-Woods, C
002916248 700__ $$aLerner, G$$uCERN
002916248 700__ $$aManna, A$$vDipartimento di Fisica e Astronomia, Università di Bologna, Italy
002916248 700__ $$aMartínez, T
002916248 700__ $$aMasi, A$$uCERN
002916248 700__ $$aMassimi, C$$vDipartimento di Fisica e Astronomia, Università di Bologna, Italy
002916248 700__ $$aMastinu, P
002916248 700__ $$aMastromarco, M$$vDipartimento Interateneo di Fisica, Università degli Studi di Bari, Italy
002916248 700__ $$aMaugeri, E A
002916248 700__ $$aMazzone, A$$vConsiglio Nazionale delle Ricerche, Bari, Italy
002916248 700__ $$aMendoza, E
002916248 700__ $$aMengoni, A$$vIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy
002916248 700__ $$aMichalopoulou, V
002916248 700__ $$aMilazzo, P M
002916248 700__ $$aMucciola, R$$vDipartimento di Fisica e Geologia, Università di Perugia, Italy
002916248 700__ $$aMurtas†, F
002916248 700__ $$aMusacchio-Gonzalez, E
002916248 700__ $$aMusumarra, A$$vDepartment of Physics and Astronomy, University of Catania, Italy
002916248 700__ $$aNegret, A
002916248 700__ $$ade Rada, A Pérez
002916248 700__ $$aPérez-Maroto, P
002916248 700__ $$aPatronis, N
002916248 700__ $$aPavón-Rodríguez, J A
002916248 700__ $$aPellegriti, M G
002916248 700__ $$aPerkowski, J
002916248 700__ $$aPetrone, C
002916248 700__ $$aPirovano, E
002916248 700__ $$aPlaza, J
002916248 700__ $$aPomp, S
002916248 700__ $$aPorras, I
002916248 700__ $$aPraena, J
002916248 700__ $$aQuesada, J M
002916248 700__ $$aReifarth, R
002916248 700__ $$aRochman, D
002916248 700__ $$aRomanets, Y
002916248 700__ $$aRubbia, C
002916248 700__ $$aSánchez-Caballero, A
002916248 700__ $$aSabaté-Gilarte, M$$uCERN
002916248 700__ $$aSchillebeeckx, P
002916248 700__ $$aSchumann, D
002916248 700__ $$aSekhar, A
002916248 700__ $$aSmith, A G
002916248 700__ $$aSosnin, N V
002916248 700__ $$aStamati, M E
002916248 700__ $$aSturniolo, A
002916248 700__ $$aTagliente, G
002916248 700__ $$aTarrío, D
002916248 700__ $$aTorres-Sánchez, P
002916248 700__ $$aVagena, E
002916248 700__ $$aValenta, S
002916248 700__ $$aVariale, V
002916248 700__ $$aVaz, P
002916248 700__ $$aVecchio, G
002916248 700__ $$aVescovi, D
002916248 700__ $$aVlachoudis, V$$uCERN
002916248 700__ $$aVlastou, R
002916248 700__ $$aWallner, A
002916248 700__ $$aWoods, P J
002916248 700__ $$aWright, T
002916248 700__ $$aZarrella, R$$vDipartimento di Fisica e Astronomia, Università di Bologna, Italy
002916248 700__ $$aŽugec, P
002916248 710__ $$gn_TOF Collaboration
002916248 773__ $$c01018$$pEPJ Web Conf.$$v284$$wC22-07-21.1$$y2023
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