D*± production by e+e- annihilation near 34.4 GeV cm energy

M. Althoff; W. Braunschweig; K. Gather; F. J. Kirschfink; K. Lübelsmeyer; H. U. Martyn; G. Peise; J. Rimkus; H. G. Sander; D. Schmitz; H. Siebke; D. Trines; W. Wallraff; H. M. Fischer; H. Hartmann; E. Hilger; W. Hillen; G. Knop; L. Köpke; H. Kolanoski; H. Kück; R. Wedemeyer; N. Wermes; M. Wollstadt; H. Burkhardt; H. Hultschig; P. Joos; W. Koch; U. Kötz; H. Kowalski; A. Ladage; B. Löhr; D. Lüke; P. Mättig; K. H. Mess; D. Notz; J. Pyrlik; D. Quarrie; R. Riethmüller; A. M. Rushton; W. Schütte; G. Wolf; G. Yekutieli; R. Fohrmann; H. L. Krasemann; P. Leu; E. Lohrmann; D. Pandoulas; G. Poelz; B. H. Wiik; I. Al-Agil; R. Beuselinck; D. M. Binnie; A. J. Campbell; P. J. Dornan; B. Foster; D. A. Garbutt; T. D. Jones; W. G. Jones; J. McCardle; J. K. Sedgbeer; K. W. Bell; M. G. Bowler; I. C. Brock; R. J. Cashmore; P. E.L. Clarke; R. Devenish; P. Grossmann; S. L. Lloyd; G. L. Salmon; J. Thomas; T. R. Wyatt; C. Youngman; J. C. Hart; J. Harvey; J. Proudfoot; D. H. Saxon; P. L. Woodworth; D. Heyland; M. Holder; M. Dittmar; E. Duchovni; Y. Eisenberg; D. Hochman; U. Karshon; G. Mikenberg; R. Mir; D. Revel; E. Ronat; A. Shapira; T. Barklow; M. Cherney; J. M. Izen; G. Rudolph; D. Strom; H. Venkataramania; E. Wicklund; Lan Wu Sau Lan Wu; G. Zobernig

doi:10.1016/0370-2693(83)90372-6

D^*± production by e⁺e^- annihilation near 34.4 GeV cm energy

M. Althoff, W. Braunschweig, K. Gather, F. J. Kirschfink, K. Lübelsmeyer, H. U. Martyn, G. Peise, J. Rimkus, H. G. Sander, D. Schmitz, H. Siebke, D. Trines, W. Wallraff, H. M. Fischer, H. Hartmann, E. Hilger, W. Hillen, G. Knop, L. Köpke, H. KolanoskiH. Kück, R. Wedemeyer, N. Wermes, M. Wollstadt, H. Burkhardt, H. Hultschig, P. Joos, W. Koch, U. Kötz, H. Kowalski, A. Ladage, B. Löhr, D. Lüke, P. Mättig, K. H. Mess, D. Notz, J. Pyrlik, D. Quarrie, R. Riethmüller, A. M. Rushton, W. Schütte, G. Wolf, G. Yekutieli, R. Fohrmann, H. L. Krasemann, P. Leu, E. Lohrmann, D. Pandoulas, G. Poelz, B. H. Wiik, I. Al-Agil, R. Beuselinck, D. M. Binnie, A. J. Campbell, P. J. Dornan, B. Foster, D. A. Garbutt, T. D. Jones, W. G. Jones, J. McCardle, J. K. Sedgbeer, K. W. Bell, M. G. Bowler, I. C. Brock, R. J. Cashmore, P. E.L. Clarke, R. Devenish, P. Grossmann, S. L. Lloyd, G. L. Salmon, J. Thomas, T. R. Wyatt, C. Youngman, J. C. Hart, J. Harvey, J. Proudfoot, D. H. Saxon, P. L. Woodworth, D. Heyland, M. Holder, M. Dittmar, E. Duchovni, Y. Eisenberg, D. Hochman, U. Karshon, G. Mikenberg, R. Mir, D. Revel, E. Ronat, A. Shapira, T. Barklow, M. Cherney, J. M. Izen, G. Rudolph, D. Strom, H. Venkataramania, E. Wicklund, Lan Wu Sau Lan Wu, G. Zobernig

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Abstract

D^*± production via e⁺e^-→D^*±X has been measured at an average CM energy of 34.4 GeV. The D^*± energy spectrum is hard, with a maximum near χ = 0.6. The size of the D^* cross section, R_D^* = σ(e⁺e^- → D^*X) σ_μμ = 2.50 ± 0.64 ± 0.88 (assuming R_D^*0 = R_D^*+) indicates that a large fraction of charm quark production yields D^* mesons. The D^*± angular distribution exhibits a forward-backward asymmetry, A = -0.28 ± 0.13. This is consistent with that expected in the standard theory for weak neutral currents and leads to |g_A ^c| = 0.89 ± 0.44 for the axial vector coupling of the charm quark.

Original language	English (US)
Pages (from-to)	493-498
Number of pages	6
Journal	Physics Letters B
Volume	126
Issue number	6
DOIs	https://doi.org/10.1016/0370-2693(83)90372-6
State	Published - Jul 14 1983
Externally published	Yes

All Science Journal Classification (ASJC) codes

Nuclear and High Energy Physics

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10.1016/0370-2693(83)90372-6

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Althoff, M., Braunschweig, W., Gather, K., Kirschfink, F. J., Lübelsmeyer, K., Martyn, H. U., Peise, G., Rimkus, J., Sander, H. G., Schmitz, D., Siebke, H., Trines, D., Wallraff, W., Fischer, H. M., Hartmann, H., Hilger, E., Hillen, W., Knop, G., Köpke, L., ... Zobernig, G. (1983). D^*± production by e⁺e^- annihilation near 34.4 GeV cm energy. Physics Letters B, 126(6), 493-498. https://doi.org/10.1016/0370-2693(83)90372-6

Althoff, M, Braunschweig, W, Gather, K, Kirschfink, FJ, Lübelsmeyer, K, Martyn, HU, Peise, G, Rimkus, J, Sander, HG, Schmitz, D, Siebke, H, Trines, D, Wallraff, W, Fischer, HM, Hartmann, H, Hilger, E, Hillen, W, Knop, G, Köpke, L, Kolanoski, H, Kück, H, Wedemeyer, R, Wermes, N, Wollstadt, M, Burkhardt, H, Hultschig, H, Joos, P, Koch, W, Kötz, U, Kowalski, H, Ladage, A, Löhr, B, Lüke, D, Mättig, P, Mess, KH, Notz, D, Pyrlik, J, Quarrie, D, Riethmüller, R, Rushton, AM, Schütte, W, Wolf, G, Yekutieli, G, Fohrmann, R, Krasemann, HL, Leu, P, Lohrmann, E, Pandoulas, D, Poelz, G, Wiik, BH, Al-Agil, I, Beuselinck, R, Binnie, DM, Campbell, AJ, Dornan, PJ, Foster, B, Garbutt, DA, Jones, TD, Jones, WG, McCardle, J, Sedgbeer, JK, Bell, KW, Bowler, MG, Brock, IC, Cashmore, RJ, Clarke, PEL, Devenish, R, Grossmann, P, Lloyd, SL, Salmon, GL, Thomas, J, Wyatt, TR, Youngman, C, Hart, JC, Harvey, J, Proudfoot, J, Saxon, DH, Woodworth, PL, Heyland, D, Holder, M, Dittmar, M, Duchovni, E, Eisenberg, Y, Hochman, D, Karshon, U, Mikenberg, G, Mir, R, Revel, D, Ronat, E, Shapira, A, Barklow, T, Cherney, M, Izen, JM, Rudolph, G, Strom, D, Venkataramania, H, Wicklund, E, Sau Lan Wu, LW & Zobernig, G 1983, 'D^*± production by e⁺e^- annihilation near 34.4 GeV cm energy', Physics Letters B, vol. 126, no. 6, pp. 493-498. https://doi.org/10.1016/0370-2693(83)90372-6

@article{fd582b2314b349d8ab3122d1c6fa461b,

title = "D*± production by e+e- annihilation near 34.4 GeV cm energy",

abstract = "D*± production via e+e-→D*±X has been measured at an average CM energy of 34.4 GeV. The D*± energy spectrum is hard, with a maximum near χ = 0.6. The size of the D* cross section, RD* = σ(e+e- → D*X) σμμ = 2.50 ± 0.64 ± 0.88 (assuming RD*0 = RD*+ ) indicates that a large fraction of charm quark production yields D* mesons. The D*± angular distribution exhibits a forward-backward asymmetry, A = -0.28 ± 0.13. This is consistent with that expected in the standard theory for weak neutral currents and leads to |gA c| = 0.89 ± 0.44 for the axial vector coupling of the charm quark.",

author = "M. Althoff and W. Braunschweig and K. Gather and Kirschfink, {F. J.} and K. L{\"u}belsmeyer and Martyn, {H. U.} and G. Peise and J. Rimkus and Sander, {H. G.} and D. Schmitz and H. Siebke and D. Trines and W. Wallraff and Fischer, {H. M.} and H. Hartmann and E. Hilger and W. Hillen and G. Knop and L. K{\"o}pke and H. Kolanoski and H. K{\"u}ck and R. Wedemeyer and N. Wermes and M. Wollstadt and H. Burkhardt and H. Hultschig and P. Joos and W. Koch and U. K{\"o}tz and H. Kowalski and A. Ladage and B. L{\"o}hr and D. L{\"u}ke and P. M{\"a}ttig and Mess, {K. H.} and D. Notz and J. Pyrlik and D. Quarrie and R. Riethm{\"u}ller and Rushton, {A. M.} and W. Sch{\"u}tte and G. Wolf and G. Yekutieli and R. Fohrmann and Krasemann, {H. L.} and P. Leu and E. Lohrmann and D. Pandoulas and G. Poelz and Wiik, {B. H.} and I. Al-Agil and R. Beuselinck and Binnie, {D. M.} and Campbell, {A. J.} and Dornan, {P. J.} and B. Foster and Garbutt, {D. A.} and Jones, {T. D.} and Jones, {W. G.} and J. McCardle and Sedgbeer, {J. K.} and Bell, {K. W.} and Bowler, {M. G.} and Brock, {I. C.} and Cashmore, {R. J.} and Clarke, {P. E.L.} and R. Devenish and P. Grossmann and Lloyd, {S. L.} and Salmon, {G. L.} and J. Thomas and Wyatt, {T. R.} and C. Youngman and Hart, {J. C.} and J. Harvey and J. Proudfoot and Saxon, {D. H.} and Woodworth, {P. L.} and D. Heyland and M. Holder and M. Dittmar and E. Duchovni and Y. Eisenberg and D. Hochman and U. Karshon and G. Mikenberg and R. Mir and D. Revel and E. Ronat and A. Shapira and T. Barklow and M. Cherney and Izen, {J. M.} and G. Rudolph and D. Strom and H. Venkataramania and E. Wicklund and {Sau Lan Wu}, {Lan Wu} and G. Zobernig",

year = "1983",

month = jul,

day = "14",

doi = "10.1016/0370-2693(83)90372-6",

language = "English (US)",

volume = "126",

pages = "493--498",

journal = "Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics",

issn = "0370-2693",

publisher = "Elsevier",

number = "6",

}

TY - JOUR

T1 - D*± production by e+e- annihilation near 34.4 GeV cm energy

AU - Althoff, M.

AU - Braunschweig, W.

AU - Gather, K.

AU - Kirschfink, F. J.

AU - Lübelsmeyer, K.

AU - Martyn, H. U.

AU - Peise, G.

AU - Rimkus, J.

AU - Sander, H. G.

AU - Schmitz, D.

AU - Siebke, H.

AU - Trines, D.

AU - Wallraff, W.

AU - Fischer, H. M.

AU - Hartmann, H.

AU - Hilger, E.

AU - Hillen, W.

AU - Knop, G.

AU - Köpke, L.

AU - Kolanoski, H.

AU - Kück, H.

AU - Wedemeyer, R.

AU - Wermes, N.

AU - Wollstadt, M.

AU - Burkhardt, H.

AU - Hultschig, H.

AU - Joos, P.

AU - Koch, W.

AU - Kötz, U.

AU - Kowalski, H.

AU - Ladage, A.

AU - Löhr, B.

AU - Lüke, D.

AU - Mättig, P.

AU - Mess, K. H.

AU - Notz, D.

AU - Pyrlik, J.

AU - Quarrie, D.

AU - Riethmüller, R.

AU - Rushton, A. M.

AU - Schütte, W.

AU - Wolf, G.

AU - Yekutieli, G.

AU - Fohrmann, R.

AU - Krasemann, H. L.

AU - Leu, P.

AU - Lohrmann, E.

AU - Pandoulas, D.

AU - Poelz, G.

AU - Wiik, B. H.

AU - Al-Agil, I.

AU - Beuselinck, R.

AU - Binnie, D. M.

AU - Campbell, A. J.

AU - Dornan, P. J.

AU - Foster, B.

AU - Garbutt, D. A.

AU - Jones, T. D.

AU - Jones, W. G.

AU - McCardle, J.

AU - Sedgbeer, J. K.

AU - Bell, K. W.

AU - Bowler, M. G.

AU - Brock, I. C.

AU - Cashmore, R. J.

AU - Clarke, P. E.L.

AU - Devenish, R.

AU - Grossmann, P.

AU - Lloyd, S. L.

AU - Salmon, G. L.

AU - Thomas, J.

AU - Wyatt, T. R.

AU - Youngman, C.

AU - Hart, J. C.

AU - Harvey, J.

AU - Proudfoot, J.

AU - Saxon, D. H.

AU - Woodworth, P. L.

AU - Heyland, D.

AU - Holder, M.

AU - Dittmar, M.

AU - Duchovni, E.

AU - Eisenberg, Y.

AU - Hochman, D.

AU - Karshon, U.

AU - Mikenberg, G.

AU - Mir, R.

AU - Revel, D.

AU - Ronat, E.

AU - Shapira, A.

AU - Barklow, T.

AU - Cherney, M.

AU - Izen, J. M.

AU - Rudolph, G.

AU - Strom, D.

AU - Venkataramania, H.

AU - Wicklund, E.

AU - Sau Lan Wu, Lan Wu

AU - Zobernig, G.

PY - 1983/7/14

Y1 - 1983/7/14

N2 - D*± production via e+e-→D*±X has been measured at an average CM energy of 34.4 GeV. The D*± energy spectrum is hard, with a maximum near χ = 0.6. The size of the D* cross section, RD* = σ(e+e- → D*X) σμμ = 2.50 ± 0.64 ± 0.88 (assuming RD*0 = RD*+ ) indicates that a large fraction of charm quark production yields D* mesons. The D*± angular distribution exhibits a forward-backward asymmetry, A = -0.28 ± 0.13. This is consistent with that expected in the standard theory for weak neutral currents and leads to |gA c| = 0.89 ± 0.44 for the axial vector coupling of the charm quark.

AB - D*± production via e+e-→D*±X has been measured at an average CM energy of 34.4 GeV. The D*± energy spectrum is hard, with a maximum near χ = 0.6. The size of the D* cross section, RD* = σ(e+e- → D*X) σμμ = 2.50 ± 0.64 ± 0.88 (assuming RD*0 = RD*+ ) indicates that a large fraction of charm quark production yields D* mesons. The D*± angular distribution exhibits a forward-backward asymmetry, A = -0.28 ± 0.13. This is consistent with that expected in the standard theory for weak neutral currents and leads to |gA c| = 0.89 ± 0.44 for the axial vector coupling of the charm quark.

UR - http://www.scopus.com/inward/record.url?scp=0040632454&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0040632454&partnerID=8YFLogxK

U2 - 10.1016/0370-2693(83)90372-6

DO - 10.1016/0370-2693(83)90372-6

M3 - Article

AN - SCOPUS:0040632454

VL - 126

SP - 493

EP - 498

JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

SN - 0370-2693

IS - 6

ER -

D^*± production by e⁺e^- annihilation near 34.4 GeV cm energy

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