Асосий контентга ўтиш
AkademIndex

Маҳсулотлар

Ишлаб чиқувчилар учун

AkademBaseЭкотизим учун очиқ API
Мақола

The<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow/><mml:mrow><mml:mn>12</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:mi>γ</mml:mi><mml:mo>,</mml:mo><mml:mi>N</mml:mi><mml:mi>N</mml:mi><mml:mo>)</mml:mo></mml:math>reaction studied over a wide kinematic range

D. P. WattsDepartment of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United KingdomI. J. D. MacGregorDepartment of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United KingdomJ. AhrensInstitut für Kernphysik, Universität Mainz, D-55099 Mainz, GermanyJ. R. M. AnnandDepartment of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United KingdomR. BeckInstitut für Kernphysik, Universität Mainz, D-55099 Mainz, GermanyD. BranfordDepartment of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3JZ, United KingdomP. GrabmayrPhysikalisches Institut, Universität Tübingen, D-72076 Tübingen, GermanyS.J. HallDepartment of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United KingdomP. D. HartyDepartment of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United KingdomT. HehlPhysikalisches Institut, Universität Tübingen, D-72076 Tübingen, GermanyJ. D. KellieDepartment of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United KingdomT. LamparterPhysikalisches Institut, Universität Tübingen, D-72076 Tübingen, GermanyM. LiangDepartment of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3JZ, United KingdomJ.A. MackenzieDepartment of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3JZ, United KingdomS. McAllisterDepartment of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United KingdomJ. C. McGeorgeDepartment of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United KingdomR.O. OwensDepartment of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United KingdomMichelle SauerPhysikalisches Institut, Universität Tübingen, D-72076 Tübingen, GermanyR. SchneiderPhysikalisches Institut, Universität Tübingen, D-72076 Tübingen, GermanyGerhard WagnerPhysikalisches Institut, Universität Tübingen, D-72076 Tübingen, GermanyT. YauDepartment of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom
2000lv
ABI

Аннотация

The ${}^{12}\mathrm{C}(\ensuremath{\gamma},np)$ and ${}^{12}\mathrm{C}(\ensuremath{\gamma},pp)$ reactions have been studied using the Glasgow photon tagging spectrometer at the Mainz MAMI electron microtron for ${E}_{\ensuremath{\gamma}}=150--700$ MeV over a kinematic range which extends well beyond the approximately back-to-back detector arrangements of previous work. For ${}^{12}\mathrm{C}(\ensuremath{\gamma},np)$ the general trends of the missing energy distributions are reproduced over a wide range of kinematics and photon energies by the theory developed by the Valencia group. The corresponding ${}^{12}\mathrm{C}(\ensuremath{\gamma},pp)$ channel is overestimated by a factor of \ensuremath{\sim}3. Detailed comparisons of the experimental data with a Monte Carlo simulation of the direct $2N$ knockout process provide the first evidence above the $\ensuremath{\Delta}$ resonance for direct $2N$ knockout and show that this process dominates the ${}^{12}\mathrm{C}(\ensuremath{\gamma},np)$ reaction at low missing energies up to ${E}_{\ensuremath{\gamma}}\ensuremath{\sim}700$ MeV. The ${}^{12}\mathrm{C}(\ensuremath{\gamma},pp)$ reaction is somewhat less well described by the Monte Carlo simulation. A possible explanation of the observed discrepancies within a direct $2N$ framework is presented. At high recoil momenta both $2N$ reaction channels exhibit an excess yield compared to the Monte Carlo prediction of direct $2N$ knockout. The excess yield in this region is compared with the predicted effects of short-range correlations and with the predicted contributions due to other reaction mechanisms.

Ҳали таржима қилинмаган

Идентификаторлар

Иқтибослар ва манбалар

1 та иқтибос0 та фойдаланилган манба