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NSR database version of May 10, 2024.

Search: Author = M.Unger

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2024AD02      Eur.Phys.J. C 84, 416 (2024)

H.Adhikary, P.Adrich, K.K.Allison, N.Amin, E.V.Andronov, T.Anticic, I.-C.Arsene, M.Bajda, Y.Balkova, M.Baszczyk, D.Battaglia, A.Bazgir, S.Bhosale, M.Bielewicz, A.Blondel, M.Bogomilov, Y.Bondar, N.Bostan, A.Brandin, W.Brylinski, J.Brzychczyk, M.Buryakov, A.F.Camino, M.Cirkovic, M.Csanad, J.Cybowska, T.Czopowicz, C.Dalmazzone, N.Davis, A.Dmitriev, P.von Doetinchem, W.Dominik, P.Dorosz, J.Dumarchez, R.Engel, G.A.Feofilov, L.Fields, Z.Fodor, M.Friend, M.Gazdzicki, O.Golosov, V.Golovatyuk, M.Golubeva, K.Grebieszkow, F.Guber, S.N.Igolkin, S.Ilieva, A.Ivashkin, A.Izvestnyy, K.Kadija, N.Kargin, N.Karpushkin, E.Kashirin, M.Kielbowicz, V.A.Kireyeu, H.Kitagawa, R.Kolesnikov, D.Kolev, Y.Koshio, V.N.Kovalenko, S.Kowalski, B.Kozlowski, A.Krasnoperov, W.Kucewicz, M.Kuchowicz, M.Kuich, A.Kurepin, A.Laszlo, M.Lewicki, G.Lykasov, V.V.Lyubushkin, M.Mackowiak-Pawlowska, Z.Majka, A.Makhnev, B.Maksiak, A.I.Malakhov, A.Marcinek, A.D.Marino, H.-J.Mathes, T.Matulewicz, V.Matveev, G.L.Melkumov, A.Merzlaya, L.Mik, A.Morawiec, S.Morozov, Y.Nagai, T.Nakadaira, M.Naskret, S.Nishimori, V.Ozvenchuk, O.Panova, V.Paolone, O.Petukhov, I.Pidhurskyi, R.Planeta, P.Podlaski, B.A.Popov, B.Porfy, M.Posiadala-Zezula, D.S.Prokhorova, D.Pszczel, S.Pulawski, J.Puzovic, R.Renfordt, L.Ren, V.Z.Reyna Ortiz, D.Rohrich, E.Rondio, M.Roth, L.Rozplochowski, B.T.Rumberger, M.Rumyantsev, A.Rustamov, M.Rybczynski, A.Rybicki, K.Sakashita, K.Schmidt, A.Yu.Seryakov, P.Seyboth, U.A.Shah, Y.Shiraishi, A.Shukla, M.Slodkowski, P.Staszel, G.Stefanek, J.Stepaniak, M.Strikhanov, H.Strobele, T.Susa, L.Swiderski, J.Szewinski, R.Szukiewicz, A.Taranenko, A.Tefelska, D.Tefelski, V.Tereshchenko, A.Toia, R.Tsenov, L.Turko, T.S.Tveter, M.Unger, M.Urbaniak, F.F.Valiev, D.Veberic, V.V.Vechernin, V.Volkov, A.Wickremasinghe, K.Wojcik, O.Wyszynski, A.Zaitsev, E.D.Zimmerman, A.Zviagina, R.Zwaska, for the NA61/SHINE collaboration

Measurements of π±, K± spectra in ⁴⁰Ar + ⁴⁵Sc collisions at 13A to 150A GeV/c

NUCLEAR REACTIONS ⁴⁵Sc(⁴⁰Ar, π), (⁴⁰Ar, K), E=13, 19, 30, 40, 75, 150 GeV/nucleon; measured reaction products; deduced inclusive double-differential spectra, transverse momentum and rapidity distributions and mean multiplicities. The NA61/SHINE experiment at the CERN Super Proton Synchrotron.

doi: 10.1140/epjc/s10052-024-12602-2
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2018GE07      Phys.Rev. C 98, 034611 (2018)

Y.Genolini, D.Maurin, I.V.Moskalenko, M.Unger

Current status and desired precision of the isotopic production cross sections relevant to astrophysics of cosmic rays: Li, Be, B, C, and N

NUCLEAR REACTIONS ¹H(¹⁰B, X), (¹¹B, X)⁶Li/⁷Li/⁹Li/⁷Be/⁹Be/¹⁰Be/¹⁰B, E=0.1-10 GeV/nucleon; ¹H(¹²C, X), (¹³C, X)⁶Li/⁷Li/⁹Li/⁷Be/⁹Be/¹⁰Be/¹⁰B/¹¹B/¹⁰C/¹¹C, E=0.1-10 GeV/nucleon; ¹H(¹⁴N, X), (¹⁵N, X)⁶Li/⁷Li/⁹Li/⁷Be/⁹Be/¹⁰Be/¹⁰B/¹¹B/¹¹C/¹²C/¹³C/¹⁴C/¹²N/¹³N/¹⁴N, E=0.1-10 GeV/nucleon; ¹H(¹⁶O, X)⁶Li/⁷Li/⁹Li/⁷Be/⁹Be/¹⁰Be/¹²Be/¹⁰B/¹¹B/¹²B/¹²C/¹³C/¹⁴C/¹²N/¹³N/¹⁴N/¹⁵N/¹³O/¹⁴O/¹⁵O, E=0.1-10 GeV/nucleon; ¹H(²⁰Ne, X), (²¹Ne, X), (²²Ne, X)¹⁰B/¹¹B/¹²B/¹⁰C/¹¹C/¹²C/¹³C/¹⁴C/¹⁵C/¹²N/¹³N/¹⁴N/¹⁵N/¹⁴O/¹⁵O/¹⁶O/¹⁸F/¹⁹F/¹⁹Ne, E=0.1-10 GeV/nucleon; ¹H(²³Na, X)¹⁵O/¹⁶O/¹⁹F, E=0.1-10 GeV/nucleon; ¹H(²⁴Mg, X), (²⁵Mg, X), (²⁶Mg, X)¹⁰B/¹¹B/¹²B/¹¹C/¹²C/¹³C/¹⁴C/¹⁵C/¹⁶C/¹²N/¹³N/¹⁴N/¹⁵N/¹⁴O/¹⁵O/¹⁶O/¹⁸F/¹⁹F/¹⁹Ne/²⁰Ne/²¹Ne/²²Ne/²²Na/²³Na/²³Mg, E=0.1-10 GeV/nucleon; ¹H(²⁷Al, X)¹⁵O/¹⁹F, E=0.1-10 GeV/nucleon; ¹H(²⁸Si, X), (²⁹Si, X)⁹Be/¹⁵O/¹⁶O/¹⁹F/¹⁹Ne/²⁰Ne/²²Na/²⁴Mg/²⁷Al/²⁷Si, E=0.1-10 GeV/nucleon; ¹H(⁵⁶Fe, X), ³⁹Ar/⁴⁰K/⁴¹K/⁴⁴Sc/⁴⁵Sc, E=0.1-10 GeV/nucleon; analyzed production σ(E) with benchmark parametrizations and compared with experimental data for the most important reaction channels for production of most astrophysically important isotopes of Li, Be, B, C, and N in cosmic ray interactions; deduced ranking of the reaction channels by their importance for a production of a particular isotope. See Supplemental Material of this paper on 52 pages for an extensive list of relevant reactions, irrespective of their flux impact on cosmic rays. Relevance to high precision modern generation cosmic-ray (CR) experiments such as AMS-02, PAMELA, CALET, ISS-CREAM, BESS-Polar, and Fermi-LAT.

doi: 10.1103/PhysRevC.98.034611
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