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arxiv: 1808.06380 · v2 · submitted 2018-08-20 · ⚛️ nucl-ex · physics.data-an· physics.ins-det

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FAMU: study of the energy dependent transfer rate Λ_{μ p rightarrow μ O}

FAMU Collaboration: E. Mocchiutti (1) , V. Bonvicini (1) , M. Danailov (1 , 2) , E. Furlanetto (1 , 3) , K. S. Gadedjisso-Tossou (1 , 4
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5) D. Guffanti (1 6) C. Pizzolotto (1) A. Rachevski (1) L. Stoychev (1 4) E. Vallazza (1) G. Zampa (1) J. Niemela (4) K. Ishida (7) A. Adamczak (8) G. Baccolo (9 10) R. Benocci (9 11) R. Bertoni (9) M. Bonesini (9) F. Chignoli (9) M. Clemenza (9 A. Curioni (9) V. Maggi (9 R. Mazza (10) M. Moretti (9 M. Nastasi (9 E. Previtali (9) D. Bakalov (12) P. Danev (12) M. Stoilov (12) G. Baldazzi (13 14) R. Campana (13) I. D'Antone (13) M. Furini (13) F. Fuschino (13 15) C. Labanti (13 A. Margotti (13) S. Meneghini (13) G. Morgante (13 L. P. Rignanese (13 P. L. Rossi (13) M. Zuffa (13) T. Cervi (16 17) A. De Bari (16 A. Menegolli (16 C. De Vecchi (17) R. Nard\`o (17) M. Rossella (17) A. Tomaselli (17 18) L. Colace (19 20) M. De Vincenzi (19 21) A. Iaciofano (19) F. Somma (19 22) L. Tortora (19) R. Ramponi (23) A. Vacchi (1 3 7) ((1) National Institute for Nuclear Physics (INFN) Sezione di Trieste via A. Valerio 2 34127 Trieste Italy (2) Elettra-Sincrotrone Trieste S.C.p.A. SS14 Km 163.5 34149 Basovizza Trieste (3) Mathematics Informatics Department Udine University via delle Scienze 206 Udine (4) The Abdus Salam International Centre for Theoretical Physics Strada Costiera 11 (5) Laboratoire de Physique des Composants \`a Semi-conducteurs (LPCS) D\'epartement de Physique Universit\'e de Lom\'e 01 BP 1515 Lom\'e Togo (6) Gran Sasso Science Institute - INFN-LNGS Via F. Crispi 7 L'Aquila (7) RIKEN-RAL RIKEN Nishina Center for Accelerator-Based Science 2-1 Hirosawa Wako Saitama 351-0198 Japan (8) Institute of Nuclear Physics Polish Academy of Sciences Radzikowskiego 152 PL31342 Krak\'o w Poland (9) National Institute for Nuclear Physics (INFN) Sezione di Milano Bicocca Piazza della Scienza 3 Milano (10) Universit\`a di Milano Bicocca Dip. di Fisica "G. Occhialini" (11) Universit\`a di Milano Bicocca Dip. di Scienze dell'Ambiente e della Terra piazza della Scienza 1 Miano (12) Institute for Nuclear Research Nuclear Energy Bulgarian Academy of Sciences blvd. Tsarigradsko ch. 72 Sofia 1142 Bulgaria (13) National Institute for Nuclear Physics (INFN) Sezione di Bologna viale Berti Pichat 6/2 Bologna (14) Department of Physics Astronomy University of Bologna (15) INAF-IAFS Bologna Area della Ricerca via P. Gobetti 101 (16) Department of Physics University of Pavia Via Bassi 6 Pavia (17) National Institute for Nuclear Physics (INFN) Sezione di Pavia (18) Department of Electrical Computer Biomedical Engineering via Ferrata 5 (19) National Institute for Nuclear Physics (INFN) Sezione di Roma Tre Via della Vasca Navale 84 Roma (20) Dipartimento di Ingegneria Universit\`a degli Studi Roma Tre via V. Volterra 62 (21) Dipartimento di Matematica e Fisica Universit\`a di Roma Tre (22) Dipartimento di Scienze viale G. Marconi 446 (23) IFN-CNR Department of Physics - Politecnico di Milano National Institute for Nuclear Physics (INFN) Sezione di Milano Politecnico piazza Leonardo da Vinci 32 20133 Milano Italy)
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classification ⚛️ nucl-ex physics.data-anphysics.ins-det
keywords energyexperimentfamuhydrogenraterightarrowtimetransfer
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The main goal of the FAMU experiment is the measurement of the hyperfine splitting (hfs) in the 1S state of muonic hydrogen $\Delta E_{hfs}(\mu^-p)1S$. The physical process behind this experiment is the following: $\mu p$ are formed in a mixture of hydrogen and a higher-Z gas. When absorbing a photon at resonance-energy $\Delta E_{hfs}\approx0.182$~eV, in subsequent collisions with the surrounding $H_2$ molecules, the $\mu p$ is quickly de-excited and accelerated by $\sim2/3$ of the excitation energy. The observable is the time distribution of the K-lines X-rays emitted from the $\mu Z$ formed by muon transfer $(\mu p) +Z \rightarrow (\mu Z)^*+p$, a reaction whose rate depends on the $\mu p$ kinetic energy. The maximal response, to the tuned laser wavelength, of the time distribution of X-ray from K-lines of the $(\mu Z)^*$ cascade indicate the resonance. During the preparatory phase of the FAMU experiment, several measurements have been performed both to validate the methodology and to prepare the best configuration of target and detectors for the spectroscopic measurement. We present here the crucial study of the energy dependence of the transfer rate from muonic hydrogen to oxygen ($\Lambda_{\mu p \rightarrow \mu O}$), precisely measured for the first time.

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