000030683 001__ 30683
000030683 005__ 20140130004616.0
000030683 037__ $$9arXiv$$aarXiv:1005.2222$$chep-ex
000030683 035__ $$9arXiv$$zoai:arXiv.org:1005.2222
000030683 037__ $$aFERMILAB-PUB-10-104-E
000030683 035__ $$9DESY$$zD10-06367
000030683 035__ $$9SPIRESTeX$$zAbazov:2010wq
000030683 100__ $$aAbazov, Victor Mukhamedovich$$iINSPIRE-00039200$$uDubna, JINR
000030683 245__ $$aSearch for scalar bottom quarks and third-generation leptoquarks in p p-bar collisions at sqrt(s) = 1.96 TeV
000030683 246__ $$9arXiv$$aSearch for scalar bottom quarks and third-generation leptoquarks in ppbar collisions at sqrt(s) = 1.96 TeV
000030683 269__ $$c2010-05
000030683 300__ $$a8
000030683 520__ $$9arXiv$$aWe report the results of a search for pair production of scalar bottom quarks (sbottom) and scalar third-generation leptoquarks in 5.2 fb-1 of ppbar collisions at the D0 experiment of the Fermilab Tevatron Collider. Scalar bottom quarks are assumed to decay to a neutralino and a $b$ quark, and we set 95% C.L. lower limits on their production in the (m_sbottom, m_neutralino) mass plane such as m_sbottom>247 GeV for m_neutralino=0 and m_neutralino>110 GeV for 160<m_sbottom<200 GeV. The leptoquarks are assumed to decay to a tau neutrino and a $b$ quark, and we set a 95% C.L. lower limit of 247 GeV on the mass of a charge-1/3 third-generation scalar leptoquark.
000030683 65017 $$2INSPIRE$$aExperiment-HEP
000030683 6507_ $$2PACS$$a14.80.-j
000030683 6507_ $$2PACS$$a13.85.Rm
000030683 6531_ $$9author$$aSupersymmetry
000030683 6531_ $$9author$$aLeptoquarks
000030683 6531_ $$9author$$aThird generation
000030683 693__ $$eFNAL-E-0823
000030683 695__ $$2INSPIRE$$aanti-p p: interaction
000030683 695__ $$2INSPIRE$$asquark: bottom
000030683 695__ $$2INSPIRE$$asquark: pair production
000030683 695__ $$2INSPIRE$$aleptoquark: pair production
000030683 695__ $$2INSPIRE$$aleptoquark: scalar
000030683 695__ $$2INSPIRE$$asquark: mass
000030683 695__ $$2INSPIRE$$aleptoquark: mass
000030683 695__ $$2INSPIRE$$afinal state: (2beauty)
000030683 695__ $$2INSPIRE$$atransverse energy: missing-energy
000030683 695__ $$2INSPIRE$$achannel cross section: branching ratio
000030683 695__ $$2INSPIRE$$aupper limit
000030683 695__ $$2INSPIRE$$aDZERO
000030683 695__ $$2INSPIRE$$aexperimental results
000030683 695__ $$2INSPIRE$$aBatavia TEVATRON Coll
000030683 695__ $$2INSPIRE$$aanti-p p --> 2squark anything
000030683 695__ $$2INSPIRE$$asquark --> beauty neutralino
000030683 695__ $$2INSPIRE$$aanti-p p --> 2leptoquark anything
000030683 695__ $$2INSPIRE$$aleptoquark --> beauty neutrino/tau
000030683 695__ $$2INSPIRE$$a1960 GeV-cms
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000030683 700__ $$aAcharya, Bannanje Sripath$$iINSPIRE-00000955$$uTata Inst.
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000030683 700__ $$aAlton, Andrew K.$$iINSPIRE-00061762$$uAugustana Coll., Sioux Falls$$uMichigan U.
000030683 700__ $$aAlverson, George O.$$iINSPIRE-00061808$$uNortheastern U.
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000030683 700__ $$aBelanger-Champagne, Camille$$iINSPIRE-00037478$$uStockholm U.
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000030683 700__ $$aBeri, Suman B.$$iINSPIRE-00045688$$uPanjab U.
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000030683 700__ $$aBeuselinck, Raymond$$iINSPIRE-00066717$$uImperial Coll., London
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000030683 700__ $$aBrooijmans, Gustaaf H.$$iINSPIRE-00069444$$uColumbia U.
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000030683 700__ $$aBurdin, Sergey$$iINSPIRE-00022855$$uLiverpool U.$$uLancaster U.
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000030683 700__ $$aCarrera, Edgar Fernando$$iINSPIRE-00009712$$uFlorida State U.
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000030683 700__ $$aChan, Kwok Ming Leo$$iINSPIRE-00032189$$uNotre Dame U.
000030683 700__ $$aChandra, Avdhesh$$iINSPIRE-00039123$$uRice U.
000030683 700__ $$aChen, Guo$$iINSPIRE-00176968$$uKansas U.
000030683 700__ $$aChevalier-Thery, Solene$$iINSPIRE-00012380$$uDAPNIA, Saclay
000030683 700__ $$aCho, DooKee$$iINSPIRE-00073093$$uBrown U.
000030683 700__ $$aCho, Sung-Woong$$iINSPIRE-00302582$$uKorea U.
000030683 700__ $$aChoi, Suyong$$iINSPIRE-00050694$$uSungkyunkwan U.
000030683 700__ $$aChoudhary, Brajesh C.$$iINSPIRE-00073233$$uDelhi U.
000030683 700__ $$aChristoudias, Theodoros$$iINSPIRE-00025069$$uImperial Coll., London
000030683 700__ $$aCihangir, Selcuk$$iINSPIRE-00073533$$uFermilab
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000030683 700__ $$aClutter, Justace Randall$$iINSPIRE-00046636$$uKansas U.
000030683 700__ $$aCooke, Michael P.$$iINSPIRE-00003477$$uFermilab
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000030683 700__ $$aCouderc, Fabrice$$iINSPIRE-00043207$$uDAPNIA, Saclay
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000030683 700__ $$aDavies, Gavin John$$iINSPIRE-00075967$$uImperial Coll., London
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000030683 700__ $$aDe La Cruz-Burelo, Eduard$$iINSPIRE-00039100$$uCINVESTAV, IPN
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000030683 700__ $$aDenisov, Dmitri S.$$iINSPIRE-00076696$$uFermilab
000030683 700__ $$aDenisov, Sergei P.$$iINSPIRE-00076710$$uSerpukhov, IHEP
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000030683 700__ $$aDiehl, H.Thomas$$iINSPIRE-00077147$$uFermilab
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000030683 700__ $$aDorland, Tyler McMillan$$iINSPIRE-00021317$$uWashington U., Seattle
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000030683 700__ $$aDudko, Lev V.$$iINSPIRE-00078338$$uMoscow State U.
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000030683 700__ $$aFisher, Wade Cameron$$iINSPIRE-00052479$$uMichigan State U.
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000030683 700__ $$aGerbaudo, Davide$$qNSPIRE-00047907$$uPrinceton U.
000030683 700__ $$aGerber, Cecilia Elena$$iINSPIRE-00084394$$uIllinois U., Chicago
000030683 700__ $$aGershtein, Yuri S.$$iINSPIRE-00058255$$uRutgers U., Piscataway
000030683 700__ $$aGillberg, Dag I.$$iINSPIRE-00006756$$uSimon Fraser U.
000030683 700__ $$aGinther, George E.Jr.$$iINSPIRE-00084917$$uRochester U.$$uFermilab
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000030683 700__ $$aGoussiou, Anna$$iINSPIRE-00086179$$uWashington U., Seattle
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000030683 700__ $$aGreder, Sebastien$$iINSPIRE-00300397$$uStrasbourg, ICS
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000030683 700__ $$aGregores, Eduardo M.$$iINSPIRE-00086681$$uABC Federal U.
000030683 700__ $$aGrenier, Gerald Jean$$iINSPIRE-00086736$$uLyon, IPN
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000030683 700__ $$aGrivaz, Jean-Francois$$iINSPIRE-00086861$$uOrsay, LAL
000030683 700__ $$aGrohsjean, Alexander$$iINSPIRE-00018559$$uDAPNIA, Saclay
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000030683 700__ $$aHall, Isaac Nathaniel$$iINSPIRE-00025373$$uMichigan State U.
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000030683 700__ $$aHarder, Kristian$$iINSPIRE-00088612$$uManchester U.
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000030683 700__ $$aHays, Jonathan M.$$iINSPIRE-00005408$$uImperial Coll., London
000030683 700__ $$aHebbeker, Thomas$$iINSPIRE-00089340$$uAachen, Tech. Hochsch.
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000030683 700__ $$aHeinson, Ann$$iINSPIRE-00089535$$uUC, Riverside
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000030683 700__ $$aHensel, Carsten$$iINSPIRE-00046890$$uGottingen U., Zweites Phys. Inst.
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000030683 700__ $$aHildreth, Michael D.$$iINSPIRE-00090190$$uNotre Dame U.
000030683 700__ $$aHirosky, Robert James$$iINSPIRE-00090388$$uVirginia U.
000030683 700__ $$aHoang, Trang$$iINSPIRE-00180370$$uFlorida State U.
000030683 700__ $$aHobbs, John D.$$iINSPIRE-00090491$$uSUNY, Stony Brook
000030683 700__ $$aHoeneisen, Bruce$$iINSPIRE-00090561$$uSan Francisco de Quito U.
000030683 700__ $$aHohlfeld, Mark$$iINSPIRE-00039005$$uMainz U., Inst. Kernphys.
000030683 700__ $$aHossain, Sohrab$$iINSPIRE-00009751$$uOklahoma U.
000030683 700__ $$aHouben, Pieter Willem$$iINSPIRE-00046459$$uNIKHEF, Amsterdam
000030683 700__ $$aHu, Yuan$$iINSPIRE-00300414$$uSUNY, Stony Brook
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000030683 700__ $$aHuske, Nils Kristian$$iINSPIRE-00019135$$uParis U., VI-VII
000030683 700__ $$aHynek, Vlastislav$$iINSPIRE-00038993$$uPrague, Tech. U.
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000030683 700__ $$aJabeen, Shabnam$$iINSPIRE-00038975$$uBrown U.
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000030683 700__ $$aJain, Supriya$$iINSPIRE-00092992$$uSUNY, Buffalo
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000030683 700__ $$aJesik, Richard L.$$iINSPIRE-00093383$$uImperial Coll., London
000030683 700__ $$aJohns, Kenneth Arthur$$iINSPIRE-00093591$$uArizona U.
000030683 700__ $$aJohnson, Chad Jeremy$$iINSPIRE-00018545$$uColumbia U.
000030683 700__ $$aJohnson, Marvin E.$$iINSPIRE-00093653$$uFermilab
000030683 700__ $$aJohnston, Dale M.$$iINSPIRE-00300436$$uNebraska U.
000030683 700__ $$aJonckheere, Alan M.$$iINSPIRE-00093762$$uFermilab
000030683 700__ $$aJonsson, Per Martin$$iINSPIRE-00093909$$uImperial Coll., London
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000030683 700__ $$aKajfasz, Eric$$iINSPIRE-00094346$$uMarseille, CPPM
000030683 700__ $$aKarmanov, Dmitriy Y.$$iINSPIRE-00000967$$uMoscow State U.
000030683 700__ $$aKasper, Penelope A.$$iINSPIRE-00095080$$uFermilab
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000030683 700__ $$aKehoe, Robert Leo Patrick III$$iINSPIRE-00095456$$uSouthern Methodist U.
000030683 700__ $$aKermiche, Smain$$iINSPIRE-00050283$$uMarseille, CPPM
000030683 700__ $$aKhalatyan, Norayr$$iINSPIRE-00032939$$uFermilab
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000030683 700__ $$aKharchilava, Avto$$iINSPIRE-00095916$$uSUNY, Buffalo
000030683 700__ $$aKharzheev, Yuri N.$$iINSPIRE-00000177$$uDubna, JINR
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000030683 700__ $$aKirby, Michael H.$$iINSPIRE-00059470$$uNorthwestern U.
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000030683 700__ $$aKozelov, Alexander V.$$iINSPIRE-00038927$$uSerpukhov, IHEP
000030683 700__ $$aKraus, James Alexander$$iINSPIRE-00025588$$uMichigan State U.
000030683 700__ $$aKumar, Ashish$$iINSPIRE-00026358$$uSUNY, Buffalo
000030683 700__ $$aKupco, Alexander$$iINSPIRE-00099163$$uPrague, Inst. Phys.
000030683 700__ $$aKurca, Tibor$$iINSPIRE-00099209$$uLyon, IPN
000030683 700__ $$aKuzmin, Valentin Alexandrovich$$iINSPIRE-00046985$$uMoscow State U.
000030683 700__ $$aKvita, Jiri$$iINSPIRE-00038915$$uCharles U.
000030683 700__ $$aLammers, Sabine Wedam$$iINSPIRE-00051670$$uIndiana U.
000030683 700__ $$aLandsberg, Greg L.$$iINSPIRE-00099870$$uBrown U.
000030683 700__ $$aLebrun, Patrice$$iINSPIRE-00100449$$uLyon, IPN
000030683 700__ $$aLee, Hyun-Su$$iINSPIRE-00302606$$uKorea U.
000030683 700__ $$aLee, William M.$$iINSPIRE-00100793$$uFermilab
000030683 700__ $$aLellouch, Jeremie$$iINSPIRE-00024906$$uParis U., VI-VII
000030683 700__ $$aLi, Liang$$iINSPIRE-00300470$$uUC, Riverside
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000030683 700__ $$aLim, Jeong ku$$iINSPIRE-00011894$$uKorea U.
000030683 700__ $$aLincoln, Donald W.$$iINSPIRE-00101920$$uFermilab
000030683 700__ $$aLinnemann, James Thomas$$iINSPIRE-00300481$$uMichigan State U.
000030683 700__ $$aLipaev, Vladimir V.$$iINSPIRE-00038891$$uSerpukhov, IHEP
000030683 700__ $$aLipton, Ronald J.$$iINSPIRE-00102104$$uFermilab
000030683 700__ $$aLiu, Yanwen$$iINSPIRE-00034400$$uHefei, CUST
000030683 700__ $$aLiu, Zhiyi$$iINSPIRE-00300492$$uSimon Fraser U.
000030683 700__ $$aLobodenko, Alexandre$$iINSPIRE-00038878$$uSt. Petersburg, INP
000030683 700__ $$aLokajicek, Milos$$iINSPIRE-00102470$$uPrague, Inst. Phys.
000030683 700__ $$aLove, Peter A.$$iINSPIRE-00006364$$uLancaster U.
000030683 700__ $$aLubatti, Henry J.$$iINSPIRE-00102893$$uWashington U., Seattle
000030683 700__ $$aLuna Garcia, Rene$$iINSPIRE-00017790$$uCIC, IPN$$uCINVESTAV, IPN
000030683 700__ $$aLyon, Adam Leonard$$iINSPIRE-00103329$$uFermilab
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000030683 700__ $$aMadar, Romain$$iINSPIRE-00301124$$uDAPNIA, Saclay
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000030683 700__ $$aMartinez-Ortega, Jorge$$iINSPIRE-00014832$$uCINVESTAV, IPN
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000030683 700__ $$aMercadante, Pedro Galli$$iINSPIRE-00106948$$uSao Paulo, IFT
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000030683 700__ $$aNeustroev, Petr V.$$iINSPIRE-00021941$$uSt. Petersburg, INP
000030683 700__ $$aNilsen, Henrik$$iINSPIRE-00300520$$uFreiburg U.
000030683 700__ $$aNovaes, Sergio F.$$iINSPIRE-00112042$$uSao Paulo, IFT
000030683 700__ $$aNunnemann, Thomas P.$$iINSPIRE-00046334$$uMunich U.
000030683 700__ $$aObrant, Gennady$$iINSPIRE-00038792$$uSt. Petersburg, INP
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000030683 700__ $$aPark, Su-Jung$$iINSPIRE-00114693$$uGottingen U., Zweites Phys. Inst.
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000030683 700__ $$aSchlobohm, Sarah Beth$$iINSPIRE-00018163$$uWashington U., Seattle
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000030683 700__ $$aSchwienhorst, Reinhard H.$$iINSPIRE-00050408$$uMichigan State U.
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000030683 710__ $$gD0 Collaboration
000030683 773__ $$a10.1016/j.physletb.2010.08.028$$c95-101$$pPhys.Lett.$$vB693$$y2010
000030683 8564_ $$uhttp://lss.fnal.gov/cgi-bin/find_paper.pl?pub-10-104$$w10-104$$yFERMILABPUB
000030683 8564_ $$uhttp://inspirebeta.net/record/855780/files/fig1.png$$y00000 (color online). The $\etmiss$ distribution before $b$-tagging. The points with the error bars represent data while the shaded histograms show the contributions from background processes. Signal distributions with ($m_{\lsb}$,$m_{\lntr}$)=(130,85)~GeV and $m_{LQ}=240$~GeV are shown as solid and dashed lines, respectively.
000030683 8564_ $$uhttp://inspirebeta.net/record/855780/files/fig2a.png$$y00001 (color online). The (a) $\etmiss$ and (b) $H_T$ distributions after $b$-tagging and additional selections. The points with the error bars represent data while the shaded histograms show the contributions from background processes. Signal distributions with ($m_{\lsb}$,$m_{\lntr}$)=(130,85)~GeV and $m_{LQ}=240$~GeV are shown as solid and dashed lines, respectively
000030683 8564_ $$uhttp://inspirebeta.net/record/855780/files/fig2b.png$$y00002 (color online). The (a) $\etmiss$ and (b) $H_T$ distributions after $b$-tagging and additional selections. The points with the error bars represent data while the shaded histograms show the contributions from background processes. Signal distributions with ($m_{\lsb}$,$m_{\lntr}$)=(130,85)~GeV and $m_{LQ}=240$~GeV are shown as solid and dashed lines, respectively
000030683 8564_ $$uhttp://inspirebeta.net/record/855780/files/fig3a.png$$y00003 (color online). (a) The 95\%~C.L. expected (dashed line) and observed (points plus solid line) limits on $\sigma \times B^2$ as a function of $m_{LQ}$ for the pair production of third-generation leptoquarks where $B$ is the branching fraction to $b\nu$. The theory band is shown in grey with an uncertainty range as discussed in the text. The long-dashed line indicates the expected suppression of $\sigma \times B^2$ above the $t\tau $ threshold for equal $b\nu $ and $t\tau $ couplings. (b) The 95\%~C.L. exclusion contour in the ($m_{\lsb}, m_{\lntr}$) plane. Also shown are results from previous searches at LEP~\cite{sboldLEP} andthe Tevatron~\cite{sboldD0,sboldCDF}.
000030683 8564_ $$uhttp://inspirebeta.net/record/855780/files/fig3b.png$$y00004 (color online). (a) The 95\%~C.L. expected (dashed line) and observed (points plus solid line) limits on $\sigma \times B^2$ as a function of $m_{LQ}$ for the pair production of third-generation leptoquarks where $B$ is the branching fraction to $b\nu$. The theory band is shown in grey with an uncertainty range as discussed in the text. The long-dashed line indicates the expected suppression of $\sigma \times B^2$ above the $t\tau $ threshold for equal $b\nu $ and $t\tau $ couplings. (b) The 95\%~C.L. exclusion contour in the ($m_{\lsb}, m_{\lntr}$) plane. Also shown are results from previous searches at LEP~\cite{sboldLEP} andthe Tevatron~\cite{sboldD0,sboldCDF}.
000030683 909CO $$ooai:jdsweb.jinr.ru:30683$$pglobal
000030683 961__ $$x2010-05-13
000030683 961__ $$c2010-10-08
000030683 970__ $$aSPIRES-8650713
000030683 980__ $$aarXiv
000030683 980__ $$aCiteable
000030683 980__ $$aCORE
000030683 999C5 $$sPhys.Rept.,117,75
000030683 999C5 $$rhep-ph/9709356
000030683 999C5 $$sPhys.Rev.Lett.,69,489
000030683 999C5 $$sAnn.Rev.Nucl.Part.Sci.,49,389
000030683 999C5 $$sPhys.Lett.,B667,1
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