Next-to-leading order QCD analysis of polarized deep inelastic scattering data
We present a next-to-leading order perturbative QCD analysis of world data on the spin dependent structure functions g 1 p , g 1 n , and g 1 d , including the new experimental information on the Q 2 dependence of g 1 n . Careful attention is paid to the experimental and theoretical uncertainties. Th...
Gespeichert in:
| Veröffentlicht in: | Physics letters. B 1997-07, Vol.405 (1), p.180-190 |
|---|---|
| Hauptverfasser: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 190 |
|---|---|
| container_issue | 1 |
| container_start_page | 180 |
| container_title | Physics letters. B |
| container_volume | 405 |
| creator | Abe, K. Akagi, T. Anderson, B.D. Anthony, P.L. Arnold, R.G. Averett, T. Band, H.R. Berisso, C.M. Bogorad, P. Borel, H. Bosted, P.E. Breton, V. Buenerd, M.J. Cates, G.D. Chupp, T.E. Churchwell, S. Coulter, K.P. Daoudi, M. Decowski, P. Erickson, R. Fellbaum, J.N. Fonvieille, H. Gearhart, R. Ghazikhanian, V. Griffioen, K.A. Hicks, R.S. Holmes, R. Hughes, E.W. Igo, G. Incerti, S. Johnson, J.R. Kahl, W. Khayat, M. Kolomensky, Yu.G. Kuhn, S.E. Kumar, K. Kuriki, M. Lombard-Nelsen, R. Manley, D.M. Marroncle, J. Maruyama, T. Marvin, T. Meyer, W. Meziani, Z.-E. Miller, D. Mitchell, G. Olson, M. Peterson, G.A. Petratos, G.G. Pitthan, R. Prepost, R. Raines, P. Raue, B.A. Reyna, D. Rochester, L.S. Rock, S.E. Romalis, M.V. Sabatie, F. Shapiro, G. Shaw, J. Smith, T.B. Sorrell, L. Souder, P.A. Staley, F. Lorant, S.St Stuart, L.M. Suekane, F. Szalata, Z.M. Terrien, Y. Thompson, A.K. Toole, T. Wang, X. Watson, J.W. Welsh, R.C. Wesselmann, F.R. Wright, T. Young, C.C. Youngman, B. Yuta, H. Zhang, W.-M. Zyla, P. |
| description | We present a next-to-leading order perturbative QCD analysis of world data on the spin dependent structure functions
g
1
p
,
g
1
n
, and
g
1
d
, including the new experimental information on the
Q
2 dependence of
g
1
n
. Careful attention is paid to the experimental and theoretical uncertainties. The data constrain the first moments of the polarized valence quark distributions, but only qualitatively constrain the polarized sea quark and gluon distributions. The NLO results are used to determine the
Q
2 dependence of the ratio
g
1
F
1
and evolve the experimental data to a constant
Q
2 = 5 GeV
2. We determine the first moments of the polarized structure functions of the proton and neutron and find agreement with the Bjorken sum rule. |
| doi_str_mv | 10.1016/S0370-2693(97)00641-2 |
| format | Article |
| fullrecord | <record><control><sourceid>hal_cross</sourceid><recordid>TN_cdi_hal_primary_oai_HAL_in2p3_00002236v1</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><els_id>S0370269397006412</els_id><sourcerecordid>oai_HAL_in2p3_00002236v1</sourcerecordid><originalsourceid>FETCH-LOGICAL-c343t-906d8f38bac224d588a494df8f1836ebd90e63999951f1e235861ab7b80b2143</originalsourceid><addsrcrecordid>eNqFkEtLAzEUhYMoWKs_QchSkWhek8mspNQnlIrYfcgkdzQyzpQkFOuvd9pKt97N3ZzvwPkQOmf0mlGmbt6oKCnhqhIXVXlJqZKM8AM0YroUhEtZHKLRPnKMTlL6pJSygqoRms_hO5PckxasD9077qOHiF-nd9h2tl2nkHDf4GXf2hh-wGMPsMShg9amHBxOzuYMcUN6m-0pOmpsm-Ds74_R4uF-MX0is5fH5-lkRpyQIpOKKq8boWvrOJe-0NrKSvpGN0wLBbWvKChRDVewhgEXhVbM1mWtac2ZFGN0tav9sK1ZxvBl49r0NpinycyEji-FGRZSzoVasSFd7NIu9ilFaPYIo2Zj0GwNmo0eU5Vma9DwgbvdcTAsWQWIJrkAnQMfIrhsfB_-afgF6Cp2oA</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Next-to-leading order QCD analysis of polarized deep inelastic scattering data</title><source>Elsevier ScienceDirect Journals</source><creator>Abe, K. ; Akagi, T. ; Anderson, B.D. ; Anthony, P.L. ; Arnold, R.G. ; Averett, T. ; Band, H.R. ; Berisso, C.M. ; Bogorad, P. ; Borel, H. ; Bosted, P.E. ; Breton, V. ; Buenerd, M.J. ; Cates, G.D. ; Chupp, T.E. ; Churchwell, S. ; Coulter, K.P. ; Daoudi, M. ; Decowski, P. ; Erickson, R. ; Fellbaum, J.N. ; Fonvieille, H. ; Gearhart, R. ; Ghazikhanian, V. ; Griffioen, K.A. ; Hicks, R.S. ; Holmes, R. ; Hughes, E.W. ; Igo, G. ; Incerti, S. ; Johnson, J.R. ; Kahl, W. ; Khayat, M. ; Kolomensky, Yu.G. ; Kuhn, S.E. ; Kumar, K. ; Kuriki, M. ; Lombard-Nelsen, R. ; Manley, D.M. ; Marroncle, J. ; Maruyama, T. ; Marvin, T. ; Meyer, W. ; Meziani, Z.-E. ; Miller, D. ; Mitchell, G. ; Olson, M. ; Peterson, G.A. ; Petratos, G.G. ; Pitthan, R. ; Prepost, R. ; Raines, P. ; Raue, B.A. ; Reyna, D. ; Rochester, L.S. ; Rock, S.E. ; Romalis, M.V. ; Sabatie, F. ; Shapiro, G. ; Shaw, J. ; Smith, T.B. ; Sorrell, L. ; Souder, P.A. ; Staley, F. ; Lorant, S.St ; Stuart, L.M. ; Suekane, F. ; Szalata, Z.M. ; Terrien, Y. ; Thompson, A.K. ; Toole, T. ; Wang, X. ; Watson, J.W. ; Welsh, R.C. ; Wesselmann, F.R. ; Wright, T. ; Young, C.C. ; Youngman, B. ; Yuta, H. ; Zhang, W.-M. ; Zyla, P.</creator><creatorcontrib>Abe, K. ; Akagi, T. ; Anderson, B.D. ; Anthony, P.L. ; Arnold, R.G. ; Averett, T. ; Band, H.R. ; Berisso, C.M. ; Bogorad, P. ; Borel, H. ; Bosted, P.E. ; Breton, V. ; Buenerd, M.J. ; Cates, G.D. ; Chupp, T.E. ; Churchwell, S. ; Coulter, K.P. ; Daoudi, M. ; Decowski, P. ; Erickson, R. ; Fellbaum, J.N. ; Fonvieille, H. ; Gearhart, R. ; Ghazikhanian, V. ; Griffioen, K.A. ; Hicks, R.S. ; Holmes, R. ; Hughes, E.W. ; Igo, G. ; Incerti, S. ; Johnson, J.R. ; Kahl, W. ; Khayat, M. ; Kolomensky, Yu.G. ; Kuhn, S.E. ; Kumar, K. ; Kuriki, M. ; Lombard-Nelsen, R. ; Manley, D.M. ; Marroncle, J. ; Maruyama, T. ; Marvin, T. ; Meyer, W. ; Meziani, Z.-E. ; Miller, D. ; Mitchell, G. ; Olson, M. ; Peterson, G.A. ; Petratos, G.G. ; Pitthan, R. ; Prepost, R. ; Raines, P. ; Raue, B.A. ; Reyna, D. ; Rochester, L.S. ; Rock, S.E. ; Romalis, M.V. ; Sabatie, F. ; Shapiro, G. ; Shaw, J. ; Smith, T.B. ; Sorrell, L. ; Souder, P.A. ; Staley, F. ; Lorant, S.St ; Stuart, L.M. ; Suekane, F. ; Szalata, Z.M. ; Terrien, Y. ; Thompson, A.K. ; Toole, T. ; Wang, X. ; Watson, J.W. ; Welsh, R.C. ; Wesselmann, F.R. ; Wright, T. ; Young, C.C. ; Youngman, B. ; Yuta, H. ; Zhang, W.-M. ; Zyla, P. ; E154 Collaboration</creatorcontrib><description>We present a next-to-leading order perturbative QCD analysis of world data on the spin dependent structure functions
g
1
p
,
g
1
n
, and
g
1
d
, including the new experimental information on the
Q
2 dependence of
g
1
n
. Careful attention is paid to the experimental and theoretical uncertainties. The data constrain the first moments of the polarized valence quark distributions, but only qualitatively constrain the polarized sea quark and gluon distributions. The NLO results are used to determine the
Q
2 dependence of the ratio
g
1
F
1
and evolve the experimental data to a constant
Q
2 = 5 GeV
2. We determine the first moments of the polarized structure functions of the proton and neutron and find agreement with the Bjorken sum rule.</description><identifier>ISSN: 0370-2693</identifier><identifier>EISSN: 1873-2445</identifier><identifier>DOI: 10.1016/S0370-2693(97)00641-2</identifier><language>eng</language><publisher>Elsevier B.V</publisher><subject>High Energy Physics - Experiment ; Physics</subject><ispartof>Physics letters. B, 1997-07, Vol.405 (1), p.180-190</ispartof><rights>1997</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c343t-906d8f38bac224d588a494df8f1836ebd90e63999951f1e235861ab7b80b2143</citedby><cites>FETCH-LOGICAL-c343t-906d8f38bac224d588a494df8f1836ebd90e63999951f1e235861ab7b80b2143</cites><orcidid>0000-0002-6908-5829 ; 0000-0001-9450-2914 ; 0000-0002-0619-2053</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.sciencedirect.com/science/article/pii/S0370269397006412$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>230,314,776,780,881,3537,27901,27902,65306</link.rule.ids><backlink>$$Uhttps://in2p3.hal.science/in2p3-00002236$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Abe, K.</creatorcontrib><creatorcontrib>Akagi, T.</creatorcontrib><creatorcontrib>Anderson, B.D.</creatorcontrib><creatorcontrib>Anthony, P.L.</creatorcontrib><creatorcontrib>Arnold, R.G.</creatorcontrib><creatorcontrib>Averett, T.</creatorcontrib><creatorcontrib>Band, H.R.</creatorcontrib><creatorcontrib>Berisso, C.M.</creatorcontrib><creatorcontrib>Bogorad, P.</creatorcontrib><creatorcontrib>Borel, H.</creatorcontrib><creatorcontrib>Bosted, P.E.</creatorcontrib><creatorcontrib>Breton, V.</creatorcontrib><creatorcontrib>Buenerd, M.J.</creatorcontrib><creatorcontrib>Cates, G.D.</creatorcontrib><creatorcontrib>Chupp, T.E.</creatorcontrib><creatorcontrib>Churchwell, S.</creatorcontrib><creatorcontrib>Coulter, K.P.</creatorcontrib><creatorcontrib>Daoudi, M.</creatorcontrib><creatorcontrib>Decowski, P.</creatorcontrib><creatorcontrib>Erickson, R.</creatorcontrib><creatorcontrib>Fellbaum, J.N.</creatorcontrib><creatorcontrib>Fonvieille, H.</creatorcontrib><creatorcontrib>Gearhart, R.</creatorcontrib><creatorcontrib>Ghazikhanian, V.</creatorcontrib><creatorcontrib>Griffioen, K.A.</creatorcontrib><creatorcontrib>Hicks, R.S.</creatorcontrib><creatorcontrib>Holmes, R.</creatorcontrib><creatorcontrib>Hughes, E.W.</creatorcontrib><creatorcontrib>Igo, G.</creatorcontrib><creatorcontrib>Incerti, S.</creatorcontrib><creatorcontrib>Johnson, J.R.</creatorcontrib><creatorcontrib>Kahl, W.</creatorcontrib><creatorcontrib>Khayat, M.</creatorcontrib><creatorcontrib>Kolomensky, Yu.G.</creatorcontrib><creatorcontrib>Kuhn, S.E.</creatorcontrib><creatorcontrib>Kumar, K.</creatorcontrib><creatorcontrib>Kuriki, M.</creatorcontrib><creatorcontrib>Lombard-Nelsen, R.</creatorcontrib><creatorcontrib>Manley, D.M.</creatorcontrib><creatorcontrib>Marroncle, J.</creatorcontrib><creatorcontrib>Maruyama, T.</creatorcontrib><creatorcontrib>Marvin, T.</creatorcontrib><creatorcontrib>Meyer, W.</creatorcontrib><creatorcontrib>Meziani, Z.-E.</creatorcontrib><creatorcontrib>Miller, D.</creatorcontrib><creatorcontrib>Mitchell, G.</creatorcontrib><creatorcontrib>Olson, M.</creatorcontrib><creatorcontrib>Peterson, G.A.</creatorcontrib><creatorcontrib>Petratos, G.G.</creatorcontrib><creatorcontrib>Pitthan, R.</creatorcontrib><creatorcontrib>Prepost, R.</creatorcontrib><creatorcontrib>Raines, P.</creatorcontrib><creatorcontrib>Raue, B.A.</creatorcontrib><creatorcontrib>Reyna, D.</creatorcontrib><creatorcontrib>Rochester, L.S.</creatorcontrib><creatorcontrib>Rock, S.E.</creatorcontrib><creatorcontrib>Romalis, M.V.</creatorcontrib><creatorcontrib>Sabatie, F.</creatorcontrib><creatorcontrib>Shapiro, G.</creatorcontrib><creatorcontrib>Shaw, J.</creatorcontrib><creatorcontrib>Smith, T.B.</creatorcontrib><creatorcontrib>Sorrell, L.</creatorcontrib><creatorcontrib>Souder, P.A.</creatorcontrib><creatorcontrib>Staley, F.</creatorcontrib><creatorcontrib>Lorant, S.St</creatorcontrib><creatorcontrib>Stuart, L.M.</creatorcontrib><creatorcontrib>Suekane, F.</creatorcontrib><creatorcontrib>Szalata, Z.M.</creatorcontrib><creatorcontrib>Terrien, Y.</creatorcontrib><creatorcontrib>Thompson, A.K.</creatorcontrib><creatorcontrib>Toole, T.</creatorcontrib><creatorcontrib>Wang, X.</creatorcontrib><creatorcontrib>Watson, J.W.</creatorcontrib><creatorcontrib>Welsh, R.C.</creatorcontrib><creatorcontrib>Wesselmann, F.R.</creatorcontrib><creatorcontrib>Wright, T.</creatorcontrib><creatorcontrib>Young, C.C.</creatorcontrib><creatorcontrib>Youngman, B.</creatorcontrib><creatorcontrib>Yuta, H.</creatorcontrib><creatorcontrib>Zhang, W.-M.</creatorcontrib><creatorcontrib>Zyla, P.</creatorcontrib><creatorcontrib>E154 Collaboration</creatorcontrib><title>Next-to-leading order QCD analysis of polarized deep inelastic scattering data</title><title>Physics letters. B</title><description>We present a next-to-leading order perturbative QCD analysis of world data on the spin dependent structure functions
g
1
p
,
g
1
n
, and
g
1
d
, including the new experimental information on the
Q
2 dependence of
g
1
n
. Careful attention is paid to the experimental and theoretical uncertainties. The data constrain the first moments of the polarized valence quark distributions, but only qualitatively constrain the polarized sea quark and gluon distributions. The NLO results are used to determine the
Q
2 dependence of the ratio
g
1
F
1
and evolve the experimental data to a constant
Q
2 = 5 GeV
2. We determine the first moments of the polarized structure functions of the proton and neutron and find agreement with the Bjorken sum rule.</description><subject>High Energy Physics - Experiment</subject><subject>Physics</subject><issn>0370-2693</issn><issn>1873-2445</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1997</creationdate><recordtype>article</recordtype><recordid>eNqFkEtLAzEUhYMoWKs_QchSkWhek8mspNQnlIrYfcgkdzQyzpQkFOuvd9pKt97N3ZzvwPkQOmf0mlGmbt6oKCnhqhIXVXlJqZKM8AM0YroUhEtZHKLRPnKMTlL6pJSygqoRms_hO5PckxasD9077qOHiF-nd9h2tl2nkHDf4GXf2hh-wGMPsMShg9amHBxOzuYMcUN6m-0pOmpsm-Ds74_R4uF-MX0is5fH5-lkRpyQIpOKKq8boWvrOJe-0NrKSvpGN0wLBbWvKChRDVewhgEXhVbM1mWtac2ZFGN0tav9sK1ZxvBl49r0NpinycyEji-FGRZSzoVasSFd7NIu9ilFaPYIo2Zj0GwNmo0eU5Vma9DwgbvdcTAsWQWIJrkAnQMfIrhsfB_-afgF6Cp2oA</recordid><startdate>19970717</startdate><enddate>19970717</enddate><creator>Abe, K.</creator><creator>Akagi, T.</creator><creator>Anderson, B.D.</creator><creator>Anthony, P.L.</creator><creator>Arnold, R.G.</creator><creator>Averett, T.</creator><creator>Band, H.R.</creator><creator>Berisso, C.M.</creator><creator>Bogorad, P.</creator><creator>Borel, H.</creator><creator>Bosted, P.E.</creator><creator>Breton, V.</creator><creator>Buenerd, M.J.</creator><creator>Cates, G.D.</creator><creator>Chupp, T.E.</creator><creator>Churchwell, S.</creator><creator>Coulter, K.P.</creator><creator>Daoudi, M.</creator><creator>Decowski, P.</creator><creator>Erickson, R.</creator><creator>Fellbaum, J.N.</creator><creator>Fonvieille, H.</creator><creator>Gearhart, R.</creator><creator>Ghazikhanian, V.</creator><creator>Griffioen, K.A.</creator><creator>Hicks, R.S.</creator><creator>Holmes, R.</creator><creator>Hughes, E.W.</creator><creator>Igo, G.</creator><creator>Incerti, S.</creator><creator>Johnson, J.R.</creator><creator>Kahl, W.</creator><creator>Khayat, M.</creator><creator>Kolomensky, Yu.G.</creator><creator>Kuhn, S.E.</creator><creator>Kumar, K.</creator><creator>Kuriki, M.</creator><creator>Lombard-Nelsen, R.</creator><creator>Manley, D.M.</creator><creator>Marroncle, J.</creator><creator>Maruyama, T.</creator><creator>Marvin, T.</creator><creator>Meyer, W.</creator><creator>Meziani, Z.-E.</creator><creator>Miller, D.</creator><creator>Mitchell, G.</creator><creator>Olson, M.</creator><creator>Peterson, G.A.</creator><creator>Petratos, G.G.</creator><creator>Pitthan, R.</creator><creator>Prepost, R.</creator><creator>Raines, P.</creator><creator>Raue, B.A.</creator><creator>Reyna, D.</creator><creator>Rochester, L.S.</creator><creator>Rock, S.E.</creator><creator>Romalis, M.V.</creator><creator>Sabatie, F.</creator><creator>Shapiro, G.</creator><creator>Shaw, J.</creator><creator>Smith, T.B.</creator><creator>Sorrell, L.</creator><creator>Souder, P.A.</creator><creator>Staley, F.</creator><creator>Lorant, S.St</creator><creator>Stuart, L.M.</creator><creator>Suekane, F.</creator><creator>Szalata, Z.M.</creator><creator>Terrien, Y.</creator><creator>Thompson, A.K.</creator><creator>Toole, T.</creator><creator>Wang, X.</creator><creator>Watson, J.W.</creator><creator>Welsh, R.C.</creator><creator>Wesselmann, F.R.</creator><creator>Wright, T.</creator><creator>Young, C.C.</creator><creator>Youngman, B.</creator><creator>Yuta, H.</creator><creator>Zhang, W.-M.</creator><creator>Zyla, P.</creator><general>Elsevier B.V</general><general>Elsevier</general><scope>AAYXX</scope><scope>CITATION</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0002-6908-5829</orcidid><orcidid>https://orcid.org/0000-0001-9450-2914</orcidid><orcidid>https://orcid.org/0000-0002-0619-2053</orcidid></search><sort><creationdate>19970717</creationdate><title>Next-to-leading order QCD analysis of polarized deep inelastic scattering data</title><author>Abe, K. ; Akagi, T. ; Anderson, B.D. ; Anthony, P.L. ; Arnold, R.G. ; Averett, T. ; Band, H.R. ; Berisso, C.M. ; Bogorad, P. ; Borel, H. ; Bosted, P.E. ; Breton, V. ; Buenerd, M.J. ; Cates, G.D. ; Chupp, T.E. ; Churchwell, S. ; Coulter, K.P. ; Daoudi, M. ; Decowski, P. ; Erickson, R. ; Fellbaum, J.N. ; Fonvieille, H. ; Gearhart, R. ; Ghazikhanian, V. ; Griffioen, K.A. ; Hicks, R.S. ; Holmes, R. ; Hughes, E.W. ; Igo, G. ; Incerti, S. ; Johnson, J.R. ; Kahl, W. ; Khayat, M. ; Kolomensky, Yu.G. ; Kuhn, S.E. ; Kumar, K. ; Kuriki, M. ; Lombard-Nelsen, R. ; Manley, D.M. ; Marroncle, J. ; Maruyama, T. ; Marvin, T. ; Meyer, W. ; Meziani, Z.-E. ; Miller, D. ; Mitchell, G. ; Olson, M. ; Peterson, G.A. ; Petratos, G.G. ; Pitthan, R. ; Prepost, R. ; Raines, P. ; Raue, B.A. ; Reyna, D. ; Rochester, L.S. ; Rock, S.E. ; Romalis, M.V. ; Sabatie, F. ; Shapiro, G. ; Shaw, J. ; Smith, T.B. ; Sorrell, L. ; Souder, P.A. ; Staley, F. ; Lorant, S.St ; Stuart, L.M. ; Suekane, F. ; Szalata, Z.M. ; Terrien, Y. ; Thompson, A.K. ; Toole, T. ; Wang, X. ; Watson, J.W. ; Welsh, R.C. ; Wesselmann, F.R. ; Wright, T. ; Young, C.C. ; Youngman, B. ; Yuta, H. ; Zhang, W.-M. ; Zyla, P.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c343t-906d8f38bac224d588a494df8f1836ebd90e63999951f1e235861ab7b80b2143</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1997</creationdate><topic>High Energy Physics - Experiment</topic><topic>Physics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Abe, K.</creatorcontrib><creatorcontrib>Akagi, T.</creatorcontrib><creatorcontrib>Anderson, B.D.</creatorcontrib><creatorcontrib>Anthony, P.L.</creatorcontrib><creatorcontrib>Arnold, R.G.</creatorcontrib><creatorcontrib>Averett, T.</creatorcontrib><creatorcontrib>Band, H.R.</creatorcontrib><creatorcontrib>Berisso, C.M.</creatorcontrib><creatorcontrib>Bogorad, P.</creatorcontrib><creatorcontrib>Borel, H.</creatorcontrib><creatorcontrib>Bosted, P.E.</creatorcontrib><creatorcontrib>Breton, V.</creatorcontrib><creatorcontrib>Buenerd, M.J.</creatorcontrib><creatorcontrib>Cates, G.D.</creatorcontrib><creatorcontrib>Chupp, T.E.</creatorcontrib><creatorcontrib>Churchwell, S.</creatorcontrib><creatorcontrib>Coulter, K.P.</creatorcontrib><creatorcontrib>Daoudi, M.</creatorcontrib><creatorcontrib>Decowski, P.</creatorcontrib><creatorcontrib>Erickson, R.</creatorcontrib><creatorcontrib>Fellbaum, J.N.</creatorcontrib><creatorcontrib>Fonvieille, H.</creatorcontrib><creatorcontrib>Gearhart, R.</creatorcontrib><creatorcontrib>Ghazikhanian, V.</creatorcontrib><creatorcontrib>Griffioen, K.A.</creatorcontrib><creatorcontrib>Hicks, R.S.</creatorcontrib><creatorcontrib>Holmes, R.</creatorcontrib><creatorcontrib>Hughes, E.W.</creatorcontrib><creatorcontrib>Igo, G.</creatorcontrib><creatorcontrib>Incerti, S.</creatorcontrib><creatorcontrib>Johnson, J.R.</creatorcontrib><creatorcontrib>Kahl, W.</creatorcontrib><creatorcontrib>Khayat, M.</creatorcontrib><creatorcontrib>Kolomensky, Yu.G.</creatorcontrib><creatorcontrib>Kuhn, S.E.</creatorcontrib><creatorcontrib>Kumar, K.</creatorcontrib><creatorcontrib>Kuriki, M.</creatorcontrib><creatorcontrib>Lombard-Nelsen, R.</creatorcontrib><creatorcontrib>Manley, D.M.</creatorcontrib><creatorcontrib>Marroncle, J.</creatorcontrib><creatorcontrib>Maruyama, T.</creatorcontrib><creatorcontrib>Marvin, T.</creatorcontrib><creatorcontrib>Meyer, W.</creatorcontrib><creatorcontrib>Meziani, Z.-E.</creatorcontrib><creatorcontrib>Miller, D.</creatorcontrib><creatorcontrib>Mitchell, G.</creatorcontrib><creatorcontrib>Olson, M.</creatorcontrib><creatorcontrib>Peterson, G.A.</creatorcontrib><creatorcontrib>Petratos, G.G.</creatorcontrib><creatorcontrib>Pitthan, R.</creatorcontrib><creatorcontrib>Prepost, R.</creatorcontrib><creatorcontrib>Raines, P.</creatorcontrib><creatorcontrib>Raue, B.A.</creatorcontrib><creatorcontrib>Reyna, D.</creatorcontrib><creatorcontrib>Rochester, L.S.</creatorcontrib><creatorcontrib>Rock, S.E.</creatorcontrib><creatorcontrib>Romalis, M.V.</creatorcontrib><creatorcontrib>Sabatie, F.</creatorcontrib><creatorcontrib>Shapiro, G.</creatorcontrib><creatorcontrib>Shaw, J.</creatorcontrib><creatorcontrib>Smith, T.B.</creatorcontrib><creatorcontrib>Sorrell, L.</creatorcontrib><creatorcontrib>Souder, P.A.</creatorcontrib><creatorcontrib>Staley, F.</creatorcontrib><creatorcontrib>Lorant, S.St</creatorcontrib><creatorcontrib>Stuart, L.M.</creatorcontrib><creatorcontrib>Suekane, F.</creatorcontrib><creatorcontrib>Szalata, Z.M.</creatorcontrib><creatorcontrib>Terrien, Y.</creatorcontrib><creatorcontrib>Thompson, A.K.</creatorcontrib><creatorcontrib>Toole, T.</creatorcontrib><creatorcontrib>Wang, X.</creatorcontrib><creatorcontrib>Watson, J.W.</creatorcontrib><creatorcontrib>Welsh, R.C.</creatorcontrib><creatorcontrib>Wesselmann, F.R.</creatorcontrib><creatorcontrib>Wright, T.</creatorcontrib><creatorcontrib>Young, C.C.</creatorcontrib><creatorcontrib>Youngman, B.</creatorcontrib><creatorcontrib>Yuta, H.</creatorcontrib><creatorcontrib>Zhang, W.-M.</creatorcontrib><creatorcontrib>Zyla, P.</creatorcontrib><creatorcontrib>E154 Collaboration</creatorcontrib><collection>CrossRef</collection><collection>Hyper Article en Ligne (HAL)</collection><jtitle>Physics letters. B</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Abe, K.</au><au>Akagi, T.</au><au>Anderson, B.D.</au><au>Anthony, P.L.</au><au>Arnold, R.G.</au><au>Averett, T.</au><au>Band, H.R.</au><au>Berisso, C.M.</au><au>Bogorad, P.</au><au>Borel, H.</au><au>Bosted, P.E.</au><au>Breton, V.</au><au>Buenerd, M.J.</au><au>Cates, G.D.</au><au>Chupp, T.E.</au><au>Churchwell, S.</au><au>Coulter, K.P.</au><au>Daoudi, M.</au><au>Decowski, P.</au><au>Erickson, R.</au><au>Fellbaum, J.N.</au><au>Fonvieille, H.</au><au>Gearhart, R.</au><au>Ghazikhanian, V.</au><au>Griffioen, K.A.</au><au>Hicks, R.S.</au><au>Holmes, R.</au><au>Hughes, E.W.</au><au>Igo, G.</au><au>Incerti, S.</au><au>Johnson, J.R.</au><au>Kahl, W.</au><au>Khayat, M.</au><au>Kolomensky, Yu.G.</au><au>Kuhn, S.E.</au><au>Kumar, K.</au><au>Kuriki, M.</au><au>Lombard-Nelsen, R.</au><au>Manley, D.M.</au><au>Marroncle, J.</au><au>Maruyama, T.</au><au>Marvin, T.</au><au>Meyer, W.</au><au>Meziani, Z.-E.</au><au>Miller, D.</au><au>Mitchell, G.</au><au>Olson, M.</au><au>Peterson, G.A.</au><au>Petratos, G.G.</au><au>Pitthan, R.</au><au>Prepost, R.</au><au>Raines, P.</au><au>Raue, B.A.</au><au>Reyna, D.</au><au>Rochester, L.S.</au><au>Rock, S.E.</au><au>Romalis, M.V.</au><au>Sabatie, F.</au><au>Shapiro, G.</au><au>Shaw, J.</au><au>Smith, T.B.</au><au>Sorrell, L.</au><au>Souder, P.A.</au><au>Staley, F.</au><au>Lorant, S.St</au><au>Stuart, L.M.</au><au>Suekane, F.</au><au>Szalata, Z.M.</au><au>Terrien, Y.</au><au>Thompson, A.K.</au><au>Toole, T.</au><au>Wang, X.</au><au>Watson, J.W.</au><au>Welsh, R.C.</au><au>Wesselmann, F.R.</au><au>Wright, T.</au><au>Young, C.C.</au><au>Youngman, B.</au><au>Yuta, H.</au><au>Zhang, W.-M.</au><au>Zyla, P.</au><aucorp>E154 Collaboration</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Next-to-leading order QCD analysis of polarized deep inelastic scattering data</atitle><jtitle>Physics letters. B</jtitle><date>1997-07-17</date><risdate>1997</risdate><volume>405</volume><issue>1</issue><spage>180</spage><epage>190</epage><pages>180-190</pages><issn>0370-2693</issn><eissn>1873-2445</eissn><abstract>We present a next-to-leading order perturbative QCD analysis of world data on the spin dependent structure functions
g
1
p
,
g
1
n
, and
g
1
d
, including the new experimental information on the
Q
2 dependence of
g
1
n
. Careful attention is paid to the experimental and theoretical uncertainties. The data constrain the first moments of the polarized valence quark distributions, but only qualitatively constrain the polarized sea quark and gluon distributions. The NLO results are used to determine the
Q
2 dependence of the ratio
g
1
F
1
and evolve the experimental data to a constant
Q
2 = 5 GeV
2. We determine the first moments of the polarized structure functions of the proton and neutron and find agreement with the Bjorken sum rule.</abstract><pub>Elsevier B.V</pub><doi>10.1016/S0370-2693(97)00641-2</doi><tpages>11</tpages><orcidid>https://orcid.org/0000-0002-6908-5829</orcidid><orcidid>https://orcid.org/0000-0001-9450-2914</orcidid><orcidid>https://orcid.org/0000-0002-0619-2053</orcidid></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0370-2693 |
| ispartof | Physics letters. B, 1997-07, Vol.405 (1), p.180-190 |
| issn | 0370-2693 1873-2445 |
| language | eng |
| recordid | cdi_hal_primary_oai_HAL_in2p3_00002236v1 |
| source | Elsevier ScienceDirect Journals |
| subjects | High Energy Physics - Experiment Physics |
| title | Next-to-leading order QCD analysis of polarized deep inelastic scattering data |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-08T12%3A18%3A09IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-hal_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Next-to-leading%20order%20QCD%20analysis%20of%20polarized%20deep%20inelastic%20scattering%20data&rft.jtitle=Physics%20letters.%20B&rft.au=Abe,%20K.&rft.aucorp=E154%20Collaboration&rft.date=1997-07-17&rft.volume=405&rft.issue=1&rft.spage=180&rft.epage=190&rft.pages=180-190&rft.issn=0370-2693&rft.eissn=1873-2445&rft_id=info:doi/10.1016/S0370-2693(97)00641-2&rft_dat=%3Chal_cross%3Eoai_HAL_in2p3_00002236v1%3C/hal_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rft_els_id=S0370269397006412&rfr_iscdi=true |