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Photoproduction of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>η</mml:mi></mml:math>-Mesic<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mrow><mml:mi>He</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mn>3</mml:mn></mml:mmultiscripts></mml:math>

M. PfeifferII. Physikalisches Institut, Universität Giessen, D-35392 Giessen, GermanyJ. AhrensInstitut für Kernphysik, Johannes-Gutenberg-Universität Mainz, D-55099 Mainz, GermanyJ. R. M. AnnandDepartment of Physics and Astronomy, University of Glasgow, Glasgow G128QQ, UKR. BeckInstitut für Kernphysik, Johannes-Gutenberg-Universität Mainz, D-55099 Mainz, GermanyG. CaselottiInstitut für Kernphysik, Johannes-Gutenberg-Universität Mainz, D-55099 Mainz, GermanyS. CherepnyaK. FöhlII. Physikalisches Institut, Universitaet Giessen, D-35392 Giessen (Germany)L. S. FogDepartment of Physics and Astronomy, University of Glasgow, Glasgow G128QQ, UKD. HornidgeInstitut für Kernphysik, Johannes-Gutenberg-Universität Mainz, D-55099 Mainz, GermanyStijn JanssenII. Physikalisches Institut, Universität Gießen, D-35392 Gießen, GermanyV. L. KashevarovP.N. Lebedev Physical Institute, Leninsky Prospect 53, 117924, Moscow, RussiaR. KondratievInstitute for Nuclear Research, 60-th October Anniversary prospect 7a, 117312, Moscow, RussiaM. KotullaInstitut fuer Kernphysik, Johannes-Gutenberg-Universitaet Mainz, D-55099 Mainz (Germany)B. KruscheDepartment of Physics and Astronomy, University of Basel, CH-4056 Basel, SwitzerlandJ. C. McGeorgeDepartment of Physics and Astronomy, University of Glasgow, Glasgow G128QQ, UKI. J. D. MacGregorDepartment of Physics and Astronomy, University of Glasgow, Glasgow G128QQ, UKK. MengelII. Physikalisches Institut, Universität Gießen, D-35392 Gießen, GermanyJ. G. MesschendorpV. MetagDepartment of Physics and Astronomy, University of Glasgow, Glasgow G128QQ, United KingdomR. NovotnyM. RostInstitut für Kernphysik, Johannes-Gutenberg-Universität Mainz, D-55099 Mainz, GermanyS. SackII. Physikalisches Institut, Universität Gießen, D-35392 Gießen, GermanyR. SandersonDepartment of Physics and Astronomy, University of Glasgow, Glasgow G128QQ, UKS. SchadmandII. Physikalisches Institut, Universitaet Giessen, D-35392 Giessen (Germany)A. ThomasInstitut fuer Kernphysik, Johannes-Gutenberg-Universitaet Mainz, D-55099 Mainz (Germany)D. P. WattsDepartment of Physics and Astronomy, University of Glasgow, Glasgow G128QQ, United Kingdom
2004lv
ABI

Аннотация

The photoproduction of $\ensuremath{\eta}$-mesic $^{3}\mathrm{He}$ has been investigated using the TAPS calorimeter at the Mainz Microtron accelerator facility MAMI. The total inclusive cross section for the reaction $\ensuremath{\gamma}^{3}\mathrm{He}\ensuremath{\rightarrow}\ensuremath{\eta}X$ has been measured for photon energies from threshold to 820 MeV. The total and angular differential coherent $\ensuremath{\eta}$ cross sections have been extracted up to energies of 745 MeV. A resonancelike structure just above the $\ensuremath{\eta}$ production threshold with an isotropic angular distribution suggests the existence of a resonant quasibound state. This is supported by studies of a competing decay channel of such a quasibound $\ensuremath{\eta}$-mesic nucleus into ${\ensuremath{\pi}}^{0}pX$. A binding energy of $(\ensuremath{-}4.4\ifmmode\pm\else\textpm\fi{}4.2)\text{ }\text{ }\mathrm{MeV}$ and a width of ($25.6\ifmmode\pm\else\textpm\fi{}6.1)\text{ }\text{ }\mathrm{MeV}$ is deduced for the quasibound $\ensuremath{\eta}$-mesic state in $^{3}\mathrm{He}$.

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