The e(+)e(-) -> p (p) over bar cross section is determined over a range of p (p) over bar masses, from threshold to 4.5 GeV/c(2), by studying the e(+)e(-)-> p (p) over bar gamma process. The data set corresponds to an integrated luminosity of 232 fb(-1), collected with the BABAR detector at the PEP-II storage ring, at an e(+)e(-) center-of-mass energy of 10.6 GeV. The mass dependence of the ratio of electric and magnetic form factors, vertical bar G(E)/G(M)vertical bar, is measured for p (p) over bar masses below 3 GeV/c(2); its value is found to be significantly larger than 1 for masses up to 2.2 GeV/c(2). We also measure J/psi -> p (p) over bar and psi(2S) -> p (p) over bar branching fractions and set an upper limit on Y(4260) -> p (p) over bar production and decay.
Study of e(+)e(-)-> p(p)over-bar using initial state radiation with BABAR / Aubert, B; Barate, R; Boutigny, D; Couderc, F; Karyotakis, Y; Lees, Jp; Poireau, V; Tisserand, V; Zghiche, A; Grauges, E; Palano, A; Pappagallo, M; Pompili, A; Chen, Jc; Qi, Nd; Rong, G; Wang, P; Zhu, Ys; Eigen, G; Ofte, I; Stugu, B; Abrams, Gs; Battaglia, M; Best, Ds; Brown, Dn; BUTTON SHAFER, J; Cahn, Rn; Charles, E; Day, Ct; Gill, Ms; Gritsan, Av; Groysman, Y; Jacobsen, Rg; Kadel, Rw; Kadyk, Ja; Kerth, Lt; Kolomensky, Yg; Kukartsev, G; Lynch, G; Mir, Lm; Oddone, Pj; Orimoto, Tj; Pripstein, M; Roe, Na; Ronan, Mt; Wenzel, Wa; Barrett, M; Ford, Ke; Harrison, Tj; Hart, Aj; Hawkes, Cm; Morgan, Se; Watson, At; Fritsch, M; Goetzen, K; Held, T; Koch, H; Lewandowski, B; Pelizaeus, M; Peters, K; Schroeder, T; Steinke, M; Boyd, Jt; Burke, Jp; Cottingham, Wn; Walker, D; CUHADAR DONSZELMANN, T; Fulsom, Bg; Hearty, C; Knecht, Ns; Mattison, Ts; Mckenna, Ja; Khan, A; Kyberd, P; Saleem, M; Teodorescu, L; Blinov, Ae; Blinov, Ve; 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Gamba, D; Bomben, M; Bosisio, L; Cartaro, C; Cossutti, F; DELLA RICCA, G; Dittongo, S; Grancagnolo, S; Lanceri, L; Vitale, L; Azzolini, V; MARTINEZ VIDAL, F; Panvini, Rs; Banerjee, S; Bhuyan, B; Brown, Cm; Fortin, D; Hamano, K; Kowalewski, R; Nugent, Im; Roney, Jm; Sobie, Rj; Back, Jj; Harrison, Pf; Latham, Te; Mohanty, Gb; Band, Hr; Chen, X; Cheng, B; Dasu, S; Datta, M; Eichenbaum, Am; Flood, Kt; Graham, Mt; Hollar, Jj; Johnson, Jr; Kutter, Pe; Li, H; Liu, R; Mellado, B; Mihalyi, A; Mohapatra, Ak; Pan, Y; Pierini, M; Prepost, R; Tan, P; Wu, Sl; Yu, Z; Neal, H.. - In: PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. - ISSN 1550-7998. - 73:(2006). [10.1103/physrevd.73.012005]
Study of e(+)e(-)-> p(p)over-bar using initial state radiation with BABAR
AUBERT B; BARATE R; BOUTIGNY D; COUDERC F; KARYOTAKIS Y; LEES JP; POIREAU V; TISSERAND V; ZGHICHE A; GRAUGES E; PALANO A; PAPPAGALLO M; POMPILI A; CHEN JC; QI ND; RONG G; WANG P; ZHU YS; EIGEN G; OFTE I; STUGU B; ABRAMS GS; BATTAGLIA M; BEST DS; BROWN DN; BUTTON SHAFER J; CAHN RN; CHARLES E; DAY CT; GILL MS; GRITSAN AV; GROYSMAN Y; JACOBSEN RG; KADEL RW; KADYK JA; KERTH LT; KOLOMENSKY YG; KUKARTSEV G; LYNCH G; MIR LM; ODDONE PJ; ORIMOTO TJ; PRIPSTEIN M; ROE NA; RONAN MT; WENZEL WA; BARRETT M; FORD KE; HARRISON TJ; HART AJ; HAWKES CM; MORGAN SE; WATSON AT; FRITSCH M; GOETZEN K; HELD T; KOCH H; LEWANDOWSKI B; PELIZAEUS M; PETERS K; SCHROEDER T; STEINKE M; BOYD JT; BURKE JP; COTTINGHAM WN; WALKER D; CUHADAR DONSZELMANN T; FULSOM BG; HEARTY C; KNECHT NS; MATTISON TS; MCKENNA JA; KHAN A; KYBERD P; SALEEM M; TEODORESCU L; BLINOV AE; BLINOV VE; BUKIN AD; DRUZHININ VP; GOLUBEV VB; KRAVCHENKO EA; ONUCHIN AP; SEREDNYAKOV SI; SKOVPEN YI; SOLODOV EP; YUSHKOV AN; BONDIOLI M; BRUINSMA M; CHAO M; CURRY S; ESCHRICH I; KIRKBY D; LANKFORD AJ; LUND P; MANDELKERN M; MOMMSEN RK; ROETHEL W; STOKER DP; ABACHI S; BUCHANAN C; FOULKES SD; GARY JW; LONG O; SHEN BC; WANG K; ZHANG L; DEL RE, Daniele ;HADAVAND HK; HILL EJ; MACFARLANE DB; PAAR HP; RAHATLOU, SHAHRAM ;SHARMA V; BERRYHILL JW; CAMPAGNARI C; CUNHA A; DAHMES B; HONG TM; MAZUR MA; RICHMAN JD; BECK TW; EISNER AM; FLACCO CJ; HEUSCH CA; KROSEBERG J; LOCKMAN WS; NESOM G; SCHALK T; SCHUMM BA; SEIDEN A; SPRADLIN P; WILLIAMS DC; WILSON MG; ALBERT J; CHEN E; DUBOIS FELSMANN GP; DVORETSKII A; HITLIN DG; MINAMORA JS; NARSKY I; PIATENKO T; PORTER FC; RYD A; SAMUEL A; ANDREASSEN R; MANCINELLI G; MEADOWS BT; SOKOLOFF MD; BLANC F; BLOOM PC; CHEN S; FORD WT; HIRSCHAUER JF; KREISEL A; NAUENBERG U; OLIVAS A; RUDDICK WO; SMITH JG; ULMER KA; WAGNER SR; ZHANG J; CHEN A; ECKHART EA; SOFFER A; TOKI WH; WILSON RJ; WINKLMEIER F; ZENG Q; ALTENBURG DD; FELTRESI E; HAUKE A; SPAAN B; BRANDT T; DICKOPP M; KLOSE V; LACKER HM; NOGOWSKI R; OTTO S; PETZOLD A; SCHUBERT J; SCHUBERT KR; SCHWIERZ R; SUNDERMANN JE; BERNARD D; BONNEAUD GR; GRENIER P; LATOUR E; SCHRENK S; THIEBAUX C; VASILEIADIS G; VERDERI M; BARD DJ; CLARK PJ; GRADL W; MUHEIM F; PLAYFER S; XIE Y; ANDREOTTI M; BETTONI D; BOZZI C; CALABRESE R; CIBINETTO G; LUPPI E; NEGRINI M; PIEMONTESE L; ANULLI F; BALDINI FERROLI R; CALCATERRA A; DE SANGRO R; FINOCCHIARO G; PATTERI P; PERUZZI IM; PICCOLO M; ZALLO A; BUZZO A; CAPRA R; CONTRI R; LO VETERE M; MACRI MM; MONGE MR; PASSAGGIO S; PATRIGNANI C; ROBUTTI E; SANTRONI A; TOSI S; BRANDENBURG G; CHAISANGUANTHUM KS; MORII M; WU J; DUBITZKY RS; MARKS J; SCHENK S; UWER U; BHIMJI W; BOWERMAN DA; DAUNCEY PD; EGEDE U; FLACK RL; GAILLARD JR; NASH JA; NIKOLICH MB; VAZQUEZ WP; CHAI X; CHARLES MJ; MADER WF; MALLIK U; ZIEGLER V; COCHRAN J; CRAWLEY HB; DONG L; EYGES V; MEYER WT; PRELL S; ROSENBERG EI; RUBIN AE; YI JI; SCHOTT G; ARNAUD N; DAVIER M; GIROUX X; GROSDIDIER G; HOCKER A; LE DIBERDER F; LEPELTIER V; LUTZ AM; OYANGUREN A; PETERSEN TC; PRUVOT S; RODIER S; ROUDEAU P; SCHUNE MH; STOCCHI A; WANG WF; WORMSER G; CHENG CH; LANGE DJ; WRIGHT DM; BEVAN AJ; CHAVEZ CA; FORSTER IJ; FRY JR; GABATHULER E; GAMET R; GEORGE KA; HUTCHCROFT DE; PARRY RJ; PAYNE DJ; SCHOFIELD KC; TOURAMANIS C; DI LODOVICO F; MENGES W; SACCO R; BROWN CL; COWAN G; FLAECHER HU; GREEN MG; HOPKINS DA; JACKSON PS; MCMAHON TR; RICCIARDI S; SALVATORE F; BROWN DN; DAVIS CL; ALLISON J; BARLOW NR; BARLOW RJ; CHIA YM; EDGAR CL; KELLY MP; LAFFERTY GD; NAISBIT MT; WILLIAMS JC; CHEN C; HULSBERGEN WD; JAWAHERY A; KOVALSKYI D; LAE CK; ROBERTS DA; SIMI G; BLAYLOCK G; DALLAPICCOLA C; HERTZBACH SS; KOFLER R; LI X; MOORE TB; SAREMI S; STAENGLE H; WILLOCQ SY; COWAN R; KOENEKE K; SCIOLLA G; SEKULA SJ; SPITZNAGEL M; TAYLOR F; YAMAMOTO RK; KIM H; PATEL PM; ROBERTSON SH; LAZZARO A; LOMBARDO V; PALOMBO FF; BAUER JM; CREMALDI L; ESCHENBURG V; GODANG R; KROEGER R; REIDY J; SANDERS DA; SUMMERS DJ; ZHAO HW; BRUNET S; COTE D; TARAS P; VIAUD FB; NICHOLSON H; CAVALLO N; DE NARDO G; FABOZZI F; GATTO C; LISTA L; MONORCHIO D; PAOLUCCI P; PICCOLO D; SCIACCA C; BAAK M; BULTEN H; RAVEN G; SNOEK HL; WILDEN L; JESSOP CP; LOSECCO JM; ALLMENDINGER T; BENELLI G; GAN KK; HONSCHEID K; HUFNAGEL D; JACKSON PD; KAGAN H; KASS R; PULLIAM T; RAHIMI AM; TER ANTONYAN R; WONG QK; BLOUNT NL; BRAU J; FREY R; IGONKINA O; LU M; POTTER CT; RAHMAT R; SINEV NB; STROM D; STRUBE J; TORRENCE E; GALEAZZI F; MARGONI M; MORANDIN M; POSOCCO M; ROTONDO M; SIMONETTO F; STROILI R; VOCI C; BENAYOUN M; CHAUVEAU J; DAVID P; DEL BUONO L; DE LA VAISSIERE C; HAMON O; HARTFIEL BL; JOHN MJJ; LERUSTE P; MALCLES J; OCARIZ J; ROOS L; THERIN G; BEHERA PK; GLADNEY L; PANETTA J; BIASINI M; COVARELLI R; PACETTI S; PIOPPI M; ANGELINI C; BATIGNANI G; BETTARINI S; BUCCI F; CALDERINI G; CARPINELLI M; CENCI R; FORTI F; GIORGI MA; LUSIANI A; MARCHIORI G; MORGANTI M; NERI N; PAOLONI E; RAMA M; RIZZO G; WALSH J; HAIRE M; JUDD D; WAGONER DE; BIESIADA J; DANIELSON N; ELMER P; LAU YP; LU C; OLSEN J; SMITH AJS; TELNOV AV; BELLINI, Fabio ;CAVOTO, Gianluca ;D'ORAZIO A; DI MARCO E; FACCINI, Riccardo ;FERRAROTTO F; FERRONI, Fernando ;GASPERO, Mario ;LI GIOI L; MAZZONI MA; MORGANTI S; PIREDDA G; POLCI F; TEHRANI FS; VOENA C ;SCHRODER H; WALDI R; ADYE T; DE GROOT N; FRANEK B; GOPAL GP; OLAIYA EO; WILSON FF; ALEKSAN R; EMERY S; GAIDOT A; GANZHUR SF; GRAZIANI G; DE MONCHENAULT GH; KOZANECKI W; LEGENDRE M; MAYER B; VASSEUR G; YECHE C; ZITO M; PUROHIT MV; WEIDEMANN AW; WILSON JR; ABE T; ALLEN MT; ASTON D; BARTOLDUS R; BERGER N; BOYARSKI AM; BUCHMUELLER OL; CLAUS R; COLEMAN JP; CONVERY MR; CRISTINZIANI M; DINGFELDER JC; DONG D; DORFAN J; DUJMIC D; DUNWOODIE W; FAN S; FIELD RC; GLANZMAN T; GOWDY SJ; HADIG T; HALYO V; HAST C; HRYN'OVA T; INNES WR; KELSEY MH; KIM P; KOCIAN ML; LEITH DWGS; LIBBY J; LUITZ S; LUTH V; LYNCH HL; MARSISKE H; MESSNER R; MULLER DR; O'GRADY CP; OZCAN VE; PERAZZO A; PERL M; RATCLIFF BN; ROODMAN A; SALNIKOV AA; SCHINDLER RH; SCHWIENING J; SNYDER A; STELZER J; SU D; SULLIVAN MK; SUZUKI K; SWAIN SK; THOMPSON JM; VA'VRA J; VAN BAKEL N; WEAVER M; WEINSTEIN AJR; WISNIEWSKI WJ; WITTGEN M; WRIGHT DH; YARRITU AK; YI K; YOUNG CC; BURCHAT PR; EDWARDS AJ; MAJEWSKI SA; PETERSEN BA; ROAT C; AHMED S; ALAM MS; BULA R; ERNST JA; PAN B; SAEED MA; WAPPLER FR; ZAIN SB; BUGG W; KRISHNAMURTHY M; SPANIER SM; ECKMANN R; RITCHIE JL; SATPATHY A; SCHWITTERS RF; IZEN JM; KITAYAMA I; LOU XC; YE S; BIANCHI F; BONA M; GALLO F; GAMBA D; BOMBEN M; BOSISIO L; CARTARO C; COSSUTTI F; DELLA RICCA G; DITTONGO S; GRANCAGNOLO S; LANCERI L; VITALE L; AZZOLINI V; MARTINEZ VIDAL F; PANVINI RS; BANERJEE S; BHUYAN B; BROWN CM; FORTIN D; HAMANO K; KOWALEWSKI R; NUGENT IM; RONEY JM; SOBIE RJ; BACK JJ; HARRISON PF; LATHAM TE; MOHANTY GB; BAND HR; CHEN X; CHENG B; DASU S; DATTA M; EICHENBAUM AM; FLOOD KT; GRAHAM MT; HOLLAR JJ; JOHNSON JR; KUTTER PE; LI H; LIU R; MELLADO B; MIHALYI A; MOHAPATRA AK; PAN Y; PIERINI M; PREPOST R; TAN P; WU SL; YU Z; NEAL H.
2006
Abstract
The e(+)e(-) -> p (p) over bar cross section is determined over a range of p (p) over bar masses, from threshold to 4.5 GeV/c(2), by studying the e(+)e(-)-> p (p) over bar gamma process. The data set corresponds to an integrated luminosity of 232 fb(-1), collected with the BABAR detector at the PEP-II storage ring, at an e(+)e(-) center-of-mass energy of 10.6 GeV. The mass dependence of the ratio of electric and magnetic form factors, vertical bar G(E)/G(M)vertical bar, is measured for p (p) over bar masses below 3 GeV/c(2); its value is found to be significantly larger than 1 for masses up to 2.2 GeV/c(2). We also measure J/psi -> p (p) over bar and psi(2S) -> p (p) over bar branching fractions and set an upper limit on Y(4260) -> p (p) over bar production and decay.
Citazione
Study of e(+)e(-)-> p(p)over-bar using initial state radiation with BABAR / Aubert, B; Barate, R; Boutigny, D; Couderc, F; Karyotakis, Y; Lees, Jp; Poireau, V; Tisserand, V; Zghiche, A; Grauges, E; Palano, A; Pappagallo, M; Pompili, A; Chen, Jc; Qi, Nd; Rong, G; Wang, P; Zhu, Ys; Eigen, G; Ofte, I; Stugu, B; Abrams, Gs; Battaglia, M; Best, Ds; Brown, Dn; BUTTON SHAFER, J; Cahn, Rn; Charles, E; Day, Ct; Gill, Ms; Gritsan, Av; Groysman, Y; Jacobsen, Rg; Kadel, Rw; Kadyk, Ja; Kerth, Lt; Kolomensky, Yg; Kukartsev, G; Lynch, G; Mir, Lm; Oddone, Pj; Orimoto, Tj; Pripstein, M; Roe, Na; Ronan, Mt; Wenzel, Wa; Barrett, M; Ford, Ke; Harrison, Tj; Hart, Aj; Hawkes, Cm; Morgan, Se; Watson, At; Fritsch, M; Goetzen, K; Held, T; Koch, H; Lewandowski, B; Pelizaeus, M; Peters, K; Schroeder, T; Steinke, M; Boyd, Jt; Burke, Jp; Cottingham, Wn; Walker, D; CUHADAR DONSZELMANN, T; Fulsom, Bg; Hearty, C; Knecht, Ns; Mattison, Ts; Mckenna, Ja; Khan, A; Kyberd, P; Saleem, M; Teodorescu, L; Blinov, Ae; Blinov, Ve; 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[10.1103/physrevd.73.012005]
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Il report seguente simula gli indicatori relativi alla propria produzione scientifica in relazione alle soglie ASN 2023-2025 del proprio SC/SSD. Si ricorda che il superamento dei valori soglia (almeno 2 su 3) è requisito necessario ma non sufficiente al conseguimento dell'abilitazione. La simulazione si basa sui dati IRIS e sugli indicatori bibliometrici alla data indicata e non tiene conto di eventuali periodi di congedo obbligatorio, che in sede di domanda ASN danno diritto a incrementi percentuali dei valori. La simulazione può differire dall'esito di un’eventuale domanda ASN sia per errori di catalogazione e/o dati mancanti in IRIS, sia per la variabilità dei dati bibliometrici nel tempo. Si consideri che Anvur calcola i valori degli indicatori all'ultima data utile per la presentazione delle domande. La presente simulazione è stata realizzata sulla base delle specifiche raccolte sul tavolo ER del Focus Group IRIS coordinato dall’Università di Modena e Reggio Emilia e delle regole riportate nel DM 589/2018 e allegata Tabella A. Cineca, l’Università di Modena e Reggio Emilia e il Focus Group IRIS non si assumono alcuna responsabilità in merito all’uso che il diretto interessato o terzi faranno della simulazione. Si specifica inoltre che la simulazione contiene calcoli effettuati con dati e algoritmi di pubblico dominio e deve quindi essere considerata come un mero ausilio al calcolo svolgibile manualmente o con strumenti equivalenti.