The OLYMPUS Experiment

Nuclear Inst. and Methods in Physics Research, A (2014) pp. 1-17 The OLYMPUS experiment was designed to measure the ratio between the positron-proton and electron-proton elastic scattering cross sections, with the goal of determining the contribution of two-photon exchange to the elastic cross secti...

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Hauptverfasser: Milner, R, Hasell, D. K, Kohl, M, Schneekloth, U, Akopov, N, Alarcon, R, Andreev, V. A, Ates, O, Avetisyan, A, Bayadilov, D, Beck, R, Belostotski, S, Bernauer, J. C, Bessuille, J, Brinker, F, Buck, B, Calarco, J. R, Carassiti, V, Cisbani, E, Ciullo, G, Contalbrigo, M, D'Ascenzo, N, De Leo, R, Diefenbach, J, Donnelly, T. W, Dow, K, Elbakian, G, Eversheim, D, Frullani, S, Funke, Ch, Gavrilov, G, Gläser, B, Görrissen, N, Hauschildt, J, Henderson, B. S, Hoffmeister, Ph, Holler, Y, Ice, L. D, Izotov, A, Kaiser, R, Karyan, G, Kelsey, J, Khaneft, D, Klassen, P, Kiselev, A, Krivshich, A, Lehmann, I, Lenisa, P, Lenz, D, Lumsden, S, Ma, Y, Maas, F, Marukyan, H, Miklukho, O, Movsisyan, A, Murray, M, Naryshkin, Y, O'Connor, C, Benito, R. Perez, Perrino, R, Redwine, R. P, Piñeiro, D. Rodríguez, Rosner, G, Russell, R. L, Schmidt, A, Seitz, B, Statera, M, Thiel, A, Vardanyan, H, Veretennikov, D, Vidal, C, Winnebeck, A, Yeganov, V
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creator Milner, R
Hasell, D. K
Kohl, M
Schneekloth, U
Akopov, N
Alarcon, R
Andreev, V. A
Ates, O
Avetisyan, A
Bayadilov, D
Beck, R
Belostotski, S
Bernauer, J. C
Bessuille, J
Brinker, F
Buck, B
Calarco, J. R
Carassiti, V
Cisbani, E
Ciullo, G
Contalbrigo, M
D'Ascenzo, N
De Leo, R
Diefenbach, J
Donnelly, T. W
Dow, K
Elbakian, G
Eversheim, D
Frullani, S
Funke, Ch
Gavrilov, G
Gläser, B
Görrissen, N
Hauschildt, J
Henderson, B. S
Hoffmeister, Ph
Holler, Y
Ice, L. D
Izotov, A
Kaiser, R
Karyan, G
Kelsey, J
Khaneft, D
Klassen, P
Kiselev, A
Krivshich, A
Lehmann, I
Lenisa, P
Lenz, D
Lumsden, S
Ma, Y
Maas, F
Marukyan, H
Miklukho, O
Movsisyan, A
Murray, M
Naryshkin, Y
O'Connor, C
Benito, R. Perez
Perrino, R
Redwine, R. P
Piñeiro, D. Rodríguez
Rosner, G
Russell, R. L
Schmidt, A
Seitz, B
Statera, M
Thiel, A
Vardanyan, H
Veretennikov, D
Vidal, C
Winnebeck, A
Yeganov, V
description Nuclear Inst. and Methods in Physics Research, A (2014) pp. 1-17 The OLYMPUS experiment was designed to measure the ratio between the positron-proton and electron-proton elastic scattering cross sections, with the goal of determining the contribution of two-photon exchange to the elastic cross section. Two-photon exchange might resolve the discrepancy between measurements of the proton form factor ratio, $\mu_p G^p_E/G^p_M$, made using polarization techniques and those made in unpolarized experiments. OLYMPUS operated on the DORIS storage ring at DESY, alternating between 2.01~GeV electron and positron beams incident on an internal hydrogen gas target. The experiment used a toroidal magnetic spectrometer instrumented with drift chambers and time-of-flight detectors to measure rates for elastic scattering over the polar angular range of approximately $25^\circ$--$75^\circ$. Symmetric M{\o}ller/Bhabha calorimeters at $1.29^\circ$ and telescopes of GEM and MWPC detectors at $12^\circ$ served as luminosity monitors. A total luminosity of approximately 4.5~fb$^{-1}$ was collected over two running periods in 2012. This paper provides details on the accelerator, target, detectors, and operation of the experiment.
doi_str_mv 10.48550/arxiv.1312.1730
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Two-photon exchange might resolve the discrepancy between measurements of the proton form factor ratio, $\mu_p G^p_E/G^p_M$, made using polarization techniques and those made in unpolarized experiments. OLYMPUS operated on the DORIS storage ring at DESY, alternating between 2.01~GeV electron and positron beams incident on an internal hydrogen gas target. The experiment used a toroidal magnetic spectrometer instrumented with drift chambers and time-of-flight detectors to measure rates for elastic scattering over the polar angular range of approximately $25^\circ$--$75^\circ$. Symmetric M{\o}ller/Bhabha calorimeters at $1.29^\circ$ and telescopes of GEM and MWPC detectors at $12^\circ$ served as luminosity monitors. A total luminosity of approximately 4.5~fb$^{-1}$ was collected over two running periods in 2012. 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P</creatorcontrib><creatorcontrib>Piñeiro, D. Rodríguez</creatorcontrib><creatorcontrib>Rosner, G</creatorcontrib><creatorcontrib>Russell, R. L</creatorcontrib><creatorcontrib>Schmidt, A</creatorcontrib><creatorcontrib>Seitz, B</creatorcontrib><creatorcontrib>Statera, M</creatorcontrib><creatorcontrib>Thiel, A</creatorcontrib><creatorcontrib>Vardanyan, H</creatorcontrib><creatorcontrib>Veretennikov, D</creatorcontrib><creatorcontrib>Vidal, C</creatorcontrib><creatorcontrib>Winnebeck, A</creatorcontrib><creatorcontrib>Yeganov, V</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Milner, R</au><au>Hasell, D. K</au><au>Kohl, M</au><au>Schneekloth, U</au><au>Akopov, N</au><au>Alarcon, R</au><au>Andreev, V. A</au><au>Ates, O</au><au>Avetisyan, A</au><au>Bayadilov, D</au><au>Beck, R</au><au>Belostotski, S</au><au>Bernauer, J. C</au><au>Bessuille, J</au><au>Brinker, F</au><au>Buck, B</au><au>Calarco, J. R</au><au>Carassiti, V</au><au>Cisbani, E</au><au>Ciullo, G</au><au>Contalbrigo, M</au><au>D'Ascenzo, N</au><au>De Leo, R</au><au>Diefenbach, J</au><au>Donnelly, T. W</au><au>Dow, K</au><au>Elbakian, G</au><au>Eversheim, D</au><au>Frullani, S</au><au>Funke, Ch</au><au>Gavrilov, G</au><au>Gläser, B</au><au>Görrissen, N</au><au>Hauschildt, J</au><au>Henderson, B. S</au><au>Hoffmeister, Ph</au><au>Holler, Y</au><au>Ice, L. D</au><au>Izotov, A</au><au>Kaiser, R</au><au>Karyan, G</au><au>Kelsey, J</au><au>Khaneft, D</au><au>Klassen, P</au><au>Kiselev, A</au><au>Krivshich, A</au><au>Lehmann, I</au><au>Lenisa, P</au><au>Lenz, D</au><au>Lumsden, S</au><au>Ma, Y</au><au>Maas, F</au><au>Marukyan, H</au><au>Miklukho, O</au><au>Movsisyan, A</au><au>Murray, M</au><au>Naryshkin, Y</au><au>O'Connor, C</au><au>Benito, R. Perez</au><au>Perrino, R</au><au>Redwine, R. P</au><au>Piñeiro, D. Rodríguez</au><au>Rosner, G</au><au>Russell, R. L</au><au>Schmidt, A</au><au>Seitz, B</au><au>Statera, M</au><au>Thiel, A</au><au>Vardanyan, H</au><au>Veretennikov, D</au><au>Vidal, C</au><au>Winnebeck, A</au><au>Yeganov, V</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The OLYMPUS Experiment</atitle><date>2013-12-05</date><risdate>2013</risdate><abstract>Nuclear Inst. and Methods in Physics Research, A (2014) pp. 1-17 The OLYMPUS experiment was designed to measure the ratio between the positron-proton and electron-proton elastic scattering cross sections, with the goal of determining the contribution of two-photon exchange to the elastic cross section. Two-photon exchange might resolve the discrepancy between measurements of the proton form factor ratio, $\mu_p G^p_E/G^p_M$, made using polarization techniques and those made in unpolarized experiments. OLYMPUS operated on the DORIS storage ring at DESY, alternating between 2.01~GeV electron and positron beams incident on an internal hydrogen gas target. The experiment used a toroidal magnetic spectrometer instrumented with drift chambers and time-of-flight detectors to measure rates for elastic scattering over the polar angular range of approximately $25^\circ$--$75^\circ$. Symmetric M{\o}ller/Bhabha calorimeters at $1.29^\circ$ and telescopes of GEM and MWPC detectors at $12^\circ$ served as luminosity monitors. A total luminosity of approximately 4.5~fb$^{-1}$ was collected over two running periods in 2012. This paper provides details on the accelerator, target, detectors, and operation of the experiment.</abstract><doi>10.48550/arxiv.1312.1730</doi><oa>free_for_read</oa></addata></record>
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identifier DOI: 10.48550/arxiv.1312.1730
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subjects Physics - Instrumentation and Detectors
Physics - Nuclear Experiment
title The OLYMPUS Experiment
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