Measurement of the WW+WZ Production Cross Section Using a Matrix Element Technique in Lepton + Jets Events

We present a measurement of the $WW+WZ$ production cross section observed in a final state consisting of an identified electron or muon, two jets, and missing transverse energy. The measurement is carried out in a data sample corresponding to up to 4.6~fb$^{-1}$ of integrated luminosity at $\sqrt{s}...

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Veröffentlicht in:Physical review. D 2010-12, Vol.82 (11)
Hauptverfasser: Aaltonen, T., Alvarez Gonzalez, B., Amerio, S., Amidei, D., Anastassov, A., Annovi, A., Antos, J., Apollinari, G., Appel, J.A., Apresyan, A., Arisawa, T., Artikov, A., Asaadi, J., Ashmanskas, W., Auerbach, B., Aurisano, A., Azfar, F., Badgett, W., Barbaro-Galtieri, A., Barnes, V.E., Barnett, B.A., Barria, P., Bartos, P., Bauce, M., Bauer, G., Bedeschi, F., Beecher, D., Behari, S., Bellettini, G., Bellinger, J., Benjamin, D., Beretvas, A., Bhatti, A., Binkley, M., Bisello, D., Bizjak, I., Bland, K.R., Blocker, C., Blumenfeld, B., Bocci, A., Bodek, A., Bortoletto, D., Boudreau, J., Boveia, A., Brau, B., Brigliadori, L., Brisuda, A., Bromberg, C., Brucken, E., Buiantonio, M., Budagov, J., Budd, H.S., Budd, S., Burkett, K., Busetto, G., Bussey, P., Buzatu, A., Cabrera, S., Calancha, C., Camarda, S., Campanelli, M., Campbell, M., Canelli, F., Canepa, A., Carls, B., Carlsmith, D., Carosi, R., Carrillo, S., Carron, S., Casal, B., Casarsa, M., Castro, A., Catastini, P., Cauz, D., Cavaliere, V., Cavalli-Sforza, M., Cerri, A., Cerrito, L., Chen, Y.C., Chertok, M., Chiarelli, G., Chlachidze, G., Chlebana, F., Cho, K., Chokheli, D., Chou, J.P., Chung, W.H., Chung, Y.S., Ciobanu, C.I., Ciocci, M.A., Clark, A., Clark, D., Compostella, G., Convery, M.E., Conway, J., Corbo, M., Cordelli, M., Cox, C.A., Cox, D.J., Crescioli, F.
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container_issue 11
container_start_page
container_title Physical review. D
container_volume 82
creator Aaltonen, T.
Alvarez Gonzalez, B.
Amerio, S.
Amidei, D.
Anastassov, A.
Annovi, A.
Antos, J.
Apollinari, G.
Appel, J.A.
Apresyan, A.
Arisawa, T.
Artikov, A.
Asaadi, J.
Ashmanskas, W.
Auerbach, B.
Aurisano, A.
Azfar, F.
Badgett, W.
Barbaro-Galtieri, A.
Barnes, V.E.
Barnett, B.A.
Barria, P.
Bartos, P.
Bauce, M.
Bauer, G.
Bedeschi, F.
Beecher, D.
Behari, S.
Bellettini, G.
Bellinger, J.
Benjamin, D.
Beretvas, A.
Bhatti, A.
Binkley, M.
Bisello, D.
Bizjak, I.
Bland, K.R.
Blocker, C.
Blumenfeld, B.
Bocci, A.
Bodek, A.
Bortoletto, D.
Boudreau, J.
Boveia, A.
Brau, B.
Brigliadori, L.
Brisuda, A.
Bromberg, C.
Brucken, E.
Buiantonio, M.
Budagov, J.
Budd, H.S.
Budd, S.
Burkett, K.
Busetto, G.
Bussey, P.
Buzatu, A.
Cabrera, S.
Calancha, C.
Camarda, S.
Campanelli, M.
Campbell, M.
Canelli, F.
Canepa, A.
Carls, B.
Carlsmith, D.
Carosi, R.
Carrillo, S.
Carron, S.
Casal, B.
Casarsa, M.
Castro, A.
Catastini, P.
Cauz, D.
Cavaliere, V.
Cavalli-Sforza, M.
Cerri, A.
Cerrito, L.
Chen, Y.C.
Chertok, M.
Chiarelli, G.
Chlachidze, G.
Chlebana, F.
Cho, K.
Chokheli, D.
Chou, J.P.
Chung, W.H.
Chung, Y.S.
Ciobanu, C.I.
Ciocci, M.A.
Clark, A.
Clark, D.
Compostella, G.
Convery, M.E.
Conway, J.
Corbo, M.
Cordelli, M.
Cox, C.A.
Cox, D.J.
Crescioli, F.
description We present a measurement of the $WW+WZ$ production cross section observed in a final state consisting of an identified electron or muon, two jets, and missing transverse energy. The measurement is carried out in a data sample corresponding to up to 4.6~fb$^{-1}$ of integrated luminosity at $\sqrt{s} = 1.96$ TeV collected by the CDF II detector. Matrix element calculations are used to separate the diboson signal from the large backgrounds. The $WW+WZ$ cross section is measured to be $17.4\pm3.3$~pb, in agreement with standard model predictions. A fit to the dijet invariant mass spectrum yields a compatible cross section measurement.
doi_str_mv 10.1103/PhysRevD.82.112001
format Article
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The measurement is carried out in a data sample corresponding to up to 4.6~fb$^{-1}$ of integrated luminosity at $\sqrt{s} = 1.96$ TeV collected by the CDF II detector. Matrix element calculations are used to separate the diboson signal from the large backgrounds. The $WW+WZ$ cross section is measured to be $17.4\pm3.3$~pb, in agreement with standard model predictions. A fit to the dijet invariant mass spectrum yields a compatible cross section measurement.</description><identifier>ISSN: 2470-0010</identifier><identifier>ISSN: 0556-2821</identifier><identifier>EISSN: 2470-0029</identifier><identifier>EISSN: 1089-4918</identifier><identifier>DOI: 10.1103/PhysRevD.82.112001</identifier><language>eng</language><publisher>United States: American Physical Society</publisher><subject>BOSONS ; CROSS SECTIONS ; ELECTRONS ; ELEMENTARY PARTICLES ; ENERGY ; ENERGY RANGE ; FERMILAB COLLIDER DETECTOR ; FERMIONS ; FIELD THEORIES ; FORECASTING ; GRAND UNIFIED THEORY ; High Energy Physics - Experiment ; INTERMEDIATE BOSONS ; INTERMEDIATE VECTOR BOSONS ; KINETIC ENERGY ; LEPTONS ; LUMINOSITY ; MASS SPECTRA ; MATHEMATICAL MODELS ; MATRIX ELEMENTS ; MEASURING INSTRUMENTS ; MUONS ; OPTICAL PROPERTIES ; PARTICLE MODELS ; PARTICLE PRODUCTION ; PHYSICAL PROPERTIES ; Physics ; PHYSICS OF ELEMENTARY PARTICLES AND FIELDS ; QUANTUM FIELD THEORY ; RADIATION DETECTORS ; SPECTRA ; STANDARD MODEL ; TEV RANGE ; TEV RANGE 01-10 ; TRANSVERSE ENERGY ; UNIFIED GAUGE MODELS ; Z NEUTRAL BOSONS</subject><ispartof>Physical review. D, 2010-12, Vol.82 (11)</ispartof><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><orcidid>0000-0002-4137-4370 ; 0000-0002-5733-5579 ; 0000-0002-2687-6380 ; 0000-0002-3655-1352 ; 0000-0002-1109-2954 ; 0000-0002-9705-5387</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885,27923,27924</link.rule.ids><backlink>$$Uhttps://in2p3.hal.science/in2p3-00515536$$DView record in HAL$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/21503707$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Aaltonen, T.</creatorcontrib><creatorcontrib>Alvarez Gonzalez, B.</creatorcontrib><creatorcontrib>Amerio, S.</creatorcontrib><creatorcontrib>Amidei, 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C.</creatorcontrib><creatorcontrib>Brucken, E.</creatorcontrib><creatorcontrib>Buiantonio, M.</creatorcontrib><creatorcontrib>Budagov, J.</creatorcontrib><creatorcontrib>Budd, H.S.</creatorcontrib><creatorcontrib>Budd, S.</creatorcontrib><creatorcontrib>Burkett, K.</creatorcontrib><creatorcontrib>Busetto, G.</creatorcontrib><creatorcontrib>Bussey, P.</creatorcontrib><creatorcontrib>Buzatu, A.</creatorcontrib><creatorcontrib>Cabrera, S.</creatorcontrib><creatorcontrib>Calancha, C.</creatorcontrib><creatorcontrib>Camarda, S.</creatorcontrib><creatorcontrib>Campanelli, M.</creatorcontrib><creatorcontrib>Campbell, M.</creatorcontrib><creatorcontrib>Canelli, F.</creatorcontrib><creatorcontrib>Canepa, A.</creatorcontrib><creatorcontrib>Carls, B.</creatorcontrib><creatorcontrib>Carlsmith, D.</creatorcontrib><creatorcontrib>Carosi, R.</creatorcontrib><creatorcontrib>Carrillo, S.</creatorcontrib><creatorcontrib>Carron, S.</creatorcontrib><creatorcontrib>Casal, B.</creatorcontrib><creatorcontrib>Casarsa, M.</creatorcontrib><creatorcontrib>Castro, A.</creatorcontrib><creatorcontrib>Catastini, P.</creatorcontrib><creatorcontrib>Cauz, D.</creatorcontrib><creatorcontrib>Cavaliere, V.</creatorcontrib><creatorcontrib>Cavalli-Sforza, M.</creatorcontrib><creatorcontrib>Cerri, A.</creatorcontrib><creatorcontrib>Cerrito, L.</creatorcontrib><creatorcontrib>Chen, Y.C.</creatorcontrib><creatorcontrib>Chertok, M.</creatorcontrib><creatorcontrib>Chiarelli, G.</creatorcontrib><creatorcontrib>Chlachidze, G.</creatorcontrib><creatorcontrib>Chlebana, F.</creatorcontrib><creatorcontrib>Cho, K.</creatorcontrib><creatorcontrib>Chokheli, D.</creatorcontrib><creatorcontrib>Chou, J.P.</creatorcontrib><creatorcontrib>Chung, W.H.</creatorcontrib><creatorcontrib>Chung, Y.S.</creatorcontrib><creatorcontrib>Ciobanu, C.I.</creatorcontrib><creatorcontrib>Ciocci, M.A.</creatorcontrib><creatorcontrib>Clark, A.</creatorcontrib><creatorcontrib>Clark, D.</creatorcontrib><creatorcontrib>Compostella, G.</creatorcontrib><creatorcontrib>Convery, M.E.</creatorcontrib><creatorcontrib>Conway, J.</creatorcontrib><creatorcontrib>Corbo, M.</creatorcontrib><creatorcontrib>Cordelli, M.</creatorcontrib><creatorcontrib>Cox, C.A.</creatorcontrib><creatorcontrib>Cox, D.J.</creatorcontrib><creatorcontrib>Crescioli, F.</creatorcontrib><title>Measurement of the WW+WZ Production Cross Section Using a Matrix Element Technique in Lepton + Jets Events</title><title>Physical review. D</title><description>We present a measurement of the $WW+WZ$ production cross section observed in a final state consisting of an identified electron or muon, two jets, and missing transverse energy. The measurement is carried out in a data sample corresponding to up to 4.6~fb$^{-1}$ of integrated luminosity at $\sqrt{s} = 1.96$ TeV collected by the CDF II detector. Matrix element calculations are used to separate the diboson signal from the large backgrounds. The $WW+WZ$ cross section is measured to be $17.4\pm3.3$~pb, in agreement with standard model predictions. A fit to the dijet invariant mass spectrum yields a compatible cross section measurement.</description><subject>BOSONS</subject><subject>CROSS SECTIONS</subject><subject>ELECTRONS</subject><subject>ELEMENTARY PARTICLES</subject><subject>ENERGY</subject><subject>ENERGY RANGE</subject><subject>FERMILAB COLLIDER DETECTOR</subject><subject>FERMIONS</subject><subject>FIELD THEORIES</subject><subject>FORECASTING</subject><subject>GRAND UNIFIED THEORY</subject><subject>High Energy Physics - Experiment</subject><subject>INTERMEDIATE BOSONS</subject><subject>INTERMEDIATE VECTOR BOSONS</subject><subject>KINETIC ENERGY</subject><subject>LEPTONS</subject><subject>LUMINOSITY</subject><subject>MASS SPECTRA</subject><subject>MATHEMATICAL MODELS</subject><subject>MATRIX ELEMENTS</subject><subject>MEASURING INSTRUMENTS</subject><subject>MUONS</subject><subject>OPTICAL PROPERTIES</subject><subject>PARTICLE MODELS</subject><subject>PARTICLE PRODUCTION</subject><subject>PHYSICAL PROPERTIES</subject><subject>Physics</subject><subject>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</subject><subject>QUANTUM FIELD THEORY</subject><subject>RADIATION DETECTORS</subject><subject>SPECTRA</subject><subject>STANDARD MODEL</subject><subject>TEV RANGE</subject><subject>TEV RANGE 01-10</subject><subject>TRANSVERSE ENERGY</subject><subject>UNIFIED GAUGE MODELS</subject><subject>Z NEUTRAL 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Society</general><scope>1XC</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0002-4137-4370</orcidid><orcidid>https://orcid.org/0000-0002-5733-5579</orcidid><orcidid>https://orcid.org/0000-0002-2687-6380</orcidid><orcidid>https://orcid.org/0000-0002-3655-1352</orcidid><orcidid>https://orcid.org/0000-0002-1109-2954</orcidid><orcidid>https://orcid.org/0000-0002-9705-5387</orcidid></search><sort><creationdate>20101201</creationdate><title>Measurement of the WW+WZ Production Cross Section Using a Matrix Element Technique in Lepton + Jets Events</title><author>Aaltonen, T. ; Alvarez Gonzalez, B. ; Amerio, S. ; Amidei, D. ; Anastassov, A. ; Annovi, A. ; Antos, J. ; Apollinari, G. ; Appel, J.A. ; Apresyan, A. ; Arisawa, T. ; Artikov, A. ; Asaadi, J. ; Ashmanskas, W. ; Auerbach, B. ; Aurisano, A. ; Azfar, F. ; Badgett, W. ; Barbaro-Galtieri, A. ; Barnes, V.E. ; Barnett, B.A. ; Barria, P. ; Bartos, P. ; Bauce, M. ; Bauer, G. ; Bedeschi, F. ; Beecher, D. ; Behari, S. ; Bellettini, G. ; Bellinger, J. ; Benjamin, D. ; Beretvas, A. ; Bhatti, A. ; Binkley, M. ; Bisello, D. ; Bizjak, I. ; Bland, K.R. ; Blocker, C. ; Blumenfeld, B. ; Bocci, A. ; Bodek, A. ; Bortoletto, D. ; Boudreau, J. ; Boveia, A. ; Brau, B. ; Brigliadori, L. ; Brisuda, A. ; Bromberg, C. ; Brucken, E. ; Buiantonio, M. ; Budagov, J. ; Budd, H.S. ; Budd, S. ; Burkett, K. ; Busetto, G. ; Bussey, P. ; Buzatu, A. ; Cabrera, S. ; Calancha, C. ; Camarda, S. ; Campanelli, M. ; Campbell, M. ; Canelli, F. ; Canepa, A. ; Carls, B. ; Carlsmith, D. ; Carosi, R. ; Carrillo, S. ; Carron, S. ; Casal, B. ; Casarsa, M. ; Castro, A. ; Catastini, P. ; Cauz, D. ; Cavaliere, V. ; Cavalli-Sforza, M. ; Cerri, A. ; Cerrito, L. ; Chen, Y.C. ; Chertok, M. ; Chiarelli, G. ; Chlachidze, G. ; Chlebana, F. ; Cho, K. ; Chokheli, D. ; Chou, J.P. ; Chung, W.H. ; Chung, Y.S. ; Ciobanu, C.I. ; Ciocci, M.A. ; Clark, A. ; Clark, D. ; Compostella, G. ; Convery, M.E. ; Conway, J. ; Corbo, M. ; Cordelli, M. ; Cox, C.A. ; Cox, D.J. ; Crescioli, F.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c170t-6848db07e8293a21dd03d2bfb5a9ba0c32370de2144000fb981d8e23a42441ce3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><topic>BOSONS</topic><topic>CROSS SECTIONS</topic><topic>ELECTRONS</topic><topic>ELEMENTARY PARTICLES</topic><topic>ENERGY</topic><topic>ENERGY RANGE</topic><topic>FERMILAB COLLIDER DETECTOR</topic><topic>FERMIONS</topic><topic>FIELD THEORIES</topic><topic>FORECASTING</topic><topic>GRAND UNIFIED THEORY</topic><topic>High Energy Physics - Experiment</topic><topic>INTERMEDIATE BOSONS</topic><topic>INTERMEDIATE VECTOR BOSONS</topic><topic>KINETIC ENERGY</topic><topic>LEPTONS</topic><topic>LUMINOSITY</topic><topic>MASS SPECTRA</topic><topic>MATHEMATICAL MODELS</topic><topic>MATRIX ELEMENTS</topic><topic>MEASURING INSTRUMENTS</topic><topic>MUONS</topic><topic>OPTICAL PROPERTIES</topic><topic>PARTICLE MODELS</topic><topic>PARTICLE PRODUCTION</topic><topic>PHYSICAL PROPERTIES</topic><topic>Physics</topic><topic>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</topic><topic>QUANTUM FIELD THEORY</topic><topic>RADIATION DETECTORS</topic><topic>SPECTRA</topic><topic>STANDARD MODEL</topic><topic>TEV RANGE</topic><topic>TEV RANGE 01-10</topic><topic>TRANSVERSE ENERGY</topic><topic>UNIFIED GAUGE MODELS</topic><topic>Z NEUTRAL BOSONS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Aaltonen, T.</creatorcontrib><creatorcontrib>Alvarez Gonzalez, B.</creatorcontrib><creatorcontrib>Amerio, S.</creatorcontrib><creatorcontrib>Amidei, D.</creatorcontrib><creatorcontrib>Anastassov, A.</creatorcontrib><creatorcontrib>Annovi, A.</creatorcontrib><creatorcontrib>Antos, J.</creatorcontrib><creatorcontrib>Apollinari, G.</creatorcontrib><creatorcontrib>Appel, J.A.</creatorcontrib><creatorcontrib>Apresyan, A.</creatorcontrib><creatorcontrib>Arisawa, 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D.J.</creatorcontrib><creatorcontrib>Crescioli, F.</creatorcontrib><collection>Hyper Article en Ligne (HAL)</collection><collection>OSTI.GOV</collection><jtitle>Physical review. D</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Aaltonen, T.</au><au>Alvarez Gonzalez, B.</au><au>Amerio, S.</au><au>Amidei, D.</au><au>Anastassov, A.</au><au>Annovi, A.</au><au>Antos, J.</au><au>Apollinari, G.</au><au>Appel, J.A.</au><au>Apresyan, A.</au><au>Arisawa, T.</au><au>Artikov, A.</au><au>Asaadi, J.</au><au>Ashmanskas, W.</au><au>Auerbach, B.</au><au>Aurisano, A.</au><au>Azfar, F.</au><au>Badgett, W.</au><au>Barbaro-Galtieri, A.</au><au>Barnes, V.E.</au><au>Barnett, B.A.</au><au>Barria, P.</au><au>Bartos, P.</au><au>Bauce, M.</au><au>Bauer, G.</au><au>Bedeschi, F.</au><au>Beecher, D.</au><au>Behari, S.</au><au>Bellettini, G.</au><au>Bellinger, J.</au><au>Benjamin, D.</au><au>Beretvas, A.</au><au>Bhatti, A.</au><au>Binkley, M.</au><au>Bisello, D.</au><au>Bizjak, I.</au><au>Bland, K.R.</au><au>Blocker, C.</au><au>Blumenfeld, B.</au><au>Bocci, A.</au><au>Bodek, A.</au><au>Bortoletto, D.</au><au>Boudreau, J.</au><au>Boveia, A.</au><au>Brau, B.</au><au>Brigliadori, L.</au><au>Brisuda, A.</au><au>Bromberg, C.</au><au>Brucken, E.</au><au>Buiantonio, M.</au><au>Budagov, J.</au><au>Budd, H.S.</au><au>Budd, S.</au><au>Burkett, K.</au><au>Busetto, G.</au><au>Bussey, P.</au><au>Buzatu, A.</au><au>Cabrera, S.</au><au>Calancha, C.</au><au>Camarda, S.</au><au>Campanelli, M.</au><au>Campbell, M.</au><au>Canelli, F.</au><au>Canepa, A.</au><au>Carls, B.</au><au>Carlsmith, D.</au><au>Carosi, R.</au><au>Carrillo, S.</au><au>Carron, S.</au><au>Casal, B.</au><au>Casarsa, M.</au><au>Castro, A.</au><au>Catastini, P.</au><au>Cauz, D.</au><au>Cavaliere, V.</au><au>Cavalli-Sforza, M.</au><au>Cerri, A.</au><au>Cerrito, L.</au><au>Chen, Y.C.</au><au>Chertok, M.</au><au>Chiarelli, G.</au><au>Chlachidze, G.</au><au>Chlebana, F.</au><au>Cho, K.</au><au>Chokheli, D.</au><au>Chou, J.P.</au><au>Chung, W.H.</au><au>Chung, Y.S.</au><au>Ciobanu, C.I.</au><au>Ciocci, M.A.</au><au>Clark, A.</au><au>Clark, D.</au><au>Compostella, G.</au><au>Convery, M.E.</au><au>Conway, J.</au><au>Corbo, M.</au><au>Cordelli, M.</au><au>Cox, C.A.</au><au>Cox, D.J.</au><au>Crescioli, F.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Measurement of the WW+WZ Production Cross Section Using a Matrix Element Technique in Lepton + Jets Events</atitle><jtitle>Physical review. D</jtitle><date>2010-12-01</date><risdate>2010</risdate><volume>82</volume><issue>11</issue><issn>2470-0010</issn><issn>0556-2821</issn><eissn>2470-0029</eissn><eissn>1089-4918</eissn><abstract>We present a measurement of the $WW+WZ$ production cross section observed in a final state consisting of an identified electron or muon, two jets, and missing transverse energy. The measurement is carried out in a data sample corresponding to up to 4.6~fb$^{-1}$ of integrated luminosity at $\sqrt{s} = 1.96$ TeV collected by the CDF II detector. Matrix element calculations are used to separate the diboson signal from the large backgrounds. The $WW+WZ$ cross section is measured to be $17.4\pm3.3$~pb, in agreement with standard model predictions. A fit to the dijet invariant mass spectrum yields a compatible cross section measurement.</abstract><cop>United States</cop><pub>American Physical Society</pub><doi>10.1103/PhysRevD.82.112001</doi><orcidid>https://orcid.org/0000-0002-4137-4370</orcidid><orcidid>https://orcid.org/0000-0002-5733-5579</orcidid><orcidid>https://orcid.org/0000-0002-2687-6380</orcidid><orcidid>https://orcid.org/0000-0002-3655-1352</orcidid><orcidid>https://orcid.org/0000-0002-1109-2954</orcidid><orcidid>https://orcid.org/0000-0002-9705-5387</orcidid></addata></record>
fulltext fulltext
identifier ISSN: 2470-0010
ispartof Physical review. D, 2010-12, Vol.82 (11)
issn 2470-0010
0556-2821
2470-0029
1089-4918
language eng
recordid cdi_osti_scitechconnect_21503707
source American Physical Society Journals
subjects BOSONS
CROSS SECTIONS
ELECTRONS
ELEMENTARY PARTICLES
ENERGY
ENERGY RANGE
FERMILAB COLLIDER DETECTOR
FERMIONS
FIELD THEORIES
FORECASTING
GRAND UNIFIED THEORY
High Energy Physics - Experiment
INTERMEDIATE BOSONS
INTERMEDIATE VECTOR BOSONS
KINETIC ENERGY
LEPTONS
LUMINOSITY
MASS SPECTRA
MATHEMATICAL MODELS
MATRIX ELEMENTS
MEASURING INSTRUMENTS
MUONS
OPTICAL PROPERTIES
PARTICLE MODELS
PARTICLE PRODUCTION
PHYSICAL PROPERTIES
Physics
PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
QUANTUM FIELD THEORY
RADIATION DETECTORS
SPECTRA
STANDARD MODEL
TEV RANGE
TEV RANGE 01-10
TRANSVERSE ENERGY
UNIFIED GAUGE MODELS
Z NEUTRAL BOSONS
title Measurement of the WW+WZ Production Cross Section Using a Matrix Element Technique in Lepton + Jets Events
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