Search for supersymmetry in the photon(s) plus missing energy channels at s\sqrt{s}=161 GeV and 172 GeV

Searches for supersymmetric particles in channels with one or more photons and missing energy have been performed with data collected by the ALEPH detector at LEP. The data consist of 11.1 \pb\ at $\sqrt{s} = 161 ~\, \rm GeV$, 1.1 \pb\ at 170 \gev\ and 9.5 \pb\ at 172 GeV. The \eenunu\ cross se ction is measured. The data are in good agreement with predictions based on the Standard Model, and are used to set upper limits on the cross sections for anomalous photon production. These limits are compared to two different SUSY models and used to set limits on the neutralino mass. A limit of 71 \gevsq\ at 95\% C.L. is set on the mass of the lightest neutralin o ($\tau_{\chi_{1}^{0}} \leq$ 3 ns) for the gauge-mediated supersymmetry breaking and LNZ models

Cosmogenic production of Ar 37 in the context of the LUX-ZEPLIN experiment

© 2022 authors. Published by the American Physical Society.We estimate the amount of Ar37 produced in natural xenon via cosmic-ray-induced spallation, an inevitable consequence of the transportation and storage of xenon on the Earth's surface. We then calculate the resulting Ar37 concentration in a 10-tonne payload (similar to that of the LUX-ZEPLIN experiment) assuming a representative schedule of xenon purification, storage, and delivery to the underground facility. Using the spallation model by Silberberg and Tsao, the sea-level production rate of Ar37 in natural xenon is estimated to be 0.024 atoms/kg/day. Assuming the xenon is successively purified to remove radioactive contaminants in 1-tonne batches at a rate of 1 tonne/month, the average Ar37 activity after 10 tons are purified and transported underground is 0.058-0.090 μBq/kg, depending on the degree of argon removal during above-ground purification. Such cosmogenic Ar37 will appear as a noticeable background in the early science data, while decaying with a 35-day half-life. This newly noticed production mechanism of Ar37 should be considered when planning for future liquid-xenon-based experiments.11Nsciescopu

SuperB Progress Reports - Detector

none240This report describes the present status of the detector design for SuperB. It is one of four separate progress reports that, taken collectively, describe progress made on the SuperB Project since the publication of the SuperB Conceptual Design Report in 2007 and the Proceedings of SuperB Workshop VI in Valencia in 2008. The other three reports relate to Physics, Accelerator and Computing.noneE. Grauges; G. Donvito; V. Spinoso; M. Manghisoni; V. Re; G. Traversi; G. Eigen; D. Fehlker; L. Helleve; A. Carbone; R. Di Sipio; A. Gabrielli; D. Galli; F. Giorgi; U. Marconi; S. Perazzini; C. Sbarra; V. Vagnoni; S. Valentinetti; M. Villa; A. Zoccoli; C. Cheng; A. Chivukula; D. Doll; B. Echenard; D. Hitlin; P. Ongmongkolkul; F. Porter; A. Rakitin; M. Thomas; R. Zhu; G. Tatishvili; R. Andreassen; C. Fabby; B. Meadows; A. Simpson; M. Sokoloff; K. Tomko; A. Fella; M. Andreotti; W. Baldini; R. Calabrese; V. Carassiti; G. Cibinetto; A. Cotta Ramusino; A. Gianoli; E. Luppi; M. Munerato; V. Santoro; L. Tomassetti; D. Stoker; O. Bezshyyko; G. Dolinska; N. Arnaud; C. Beigbeder; F. Bogard; D. Breton; L. Burmistrov; D. Charlet; J. Maalmi; L. Perez; V. Puill; A. Stocchi; V. Tocut; S. Wallon; G. Wormser; D. Brown; A. Calcaterra; R. de Sangro; G. Felici; G. Finocchiaro; P. Patteri; I. Peruzzi; M. Piccolo; M. Rama; S. Fantinel; G. Maron; E. Ben-Haim; G. Calderini; H. Lebbolo; G. Marchiori; R. Cenci; A. Jawahery; D.A. Roberts; D. Lindemann; P. Patel; S. Robertson; D. Swersky; P. Biassoni; M. Citterio; V. Liberali; F. Palombo; A. Stabile; S. Stracka; A. Aloisio; S. Cavaliere; G. De Nardo; A. Doria; R. Giordano; A. Ordine; S. Pardi; G. Russo; C. Sciacca; A.Y. Barniakov; M.Y. Barniakov; V.E. Blinov; V.P. Druzhinin; V.B.. Golubev; S.A. Kononov; E. Kravchenko; A.P. Onuchin; S.I. Serednyakov; Y.I. Skovpen; E.P. Solodov; M. Bellato; M. Benettoni; M. Corvo; A. Crescente; F. Dal Corso; C. Fanin; E. Feltresi; N. Gagliardi; M. Morandin; M. Posocco; M. Rotondo; R. Stroili; C. Andreoli; L. Gaioni; E. Pozzati; L. Ratti; V. Speziali; D. Aisa; M. Bizzarri; C. Cecchi; S. Germani; P. Lubrano; E. Manoni; A. Papi; A. Piluso ; A. Rossi; M. Lebeau; C. Avanzini; G. Batignani; S. Bettarini; F. Bosi; M. Ceccanti; A. Cervelli; A. Ciampa; F. Crescioli; M. Dell’Orso; D. Fabiani; F. Forti; P. Giannetti; M. Giorgi; S. Gregucci; A. Lusiani; P. Mammini; G. Marchiori; M. Massa; E. Mazzoni; F. Morsani; N. Neri; E. Paoloni; E. Paoloni; M. Piendibene; A. Profeti; G. Rizzo; L. Sartori; J. Walsh; E. Yurtsev; D.M. Asner; J. E. Fast; R.T. Kouzes; A. Bevan; F. Gannaway; J. Mistry; C. Walker; C.A.J. Brew; R.E. Coath; J.P. Crooks; R.M. Harper; A. Lintern; A. Nichols; M. Staniztki; R. Turchetta; F.F. Wilson; V. Bocci; G. Chiodi; R. Faccini; C. Gargiulo; D. Pinci; L. Recchia; D. Ruggieri; A. Di Simone; P. Branchini; A. Passeri; F. Ruggieri; E. Spiriti; D. Aston; M. Convery; G. Dubois-Felsmann; W. Dunwoodie; M. Kelsey; P. Kim; M. Kocian; D. Leith; S. Luitz; D. MacFarlane; B. Ratcliff; M. Sullivan; J. Va’vra; W. Wisniewski; W. Yang; K. Shougaev; A. Soffer; F. Bianchi; D. Gamba; G. Giraudo; P. Mereu; G. Dalla Betta; G. Fontana; G. Soncini; M. Bomben; L. Bosisio; P. Cristaudo; G. Giacomini; D. Jugovaz; L. Lanceri; I. Rashevskaya; G. Venier; L. Vitale; R. Henderson; J.-F. Caron; C. Hearty; P. Lu; R. So; P. Taras; A. Agarwal; J. Franta; J.M. RoneyE., Grauges; G., Donvito; V., Spinoso; M., Manghisoni; V., Re; G., Traversi; G., Eigen; D., Fehlker; L., Helleve; A., Carbone; R., Di Sipio; A., Gabrielli; D., Galli; F., Giorgi; U., Marconi; S., Perazzini; C., Sbarra; V., Vagnoni; S., Valentinetti; M., Villa; A., Zoccoli; C., Cheng; A., Chivukula; D., Doll; B., Echenard; D., Hitlin; P., Ongmongkolkul; F., Porter; A., Rakitin; M., Thomas; R., Zhu; G., Tatishvili; R., Andreassen; C., Fabby; B., Meadows; A., Simpson; M., Sokoloff; K., Tomko; A., Fella; Andreotti, Mirco; Baldini, Wander; Calabrese, Roberto; Carassiti, Vittore; Cibinetto, Gianluigi; COTTA RAMUSINO, Angelo; Gianoli, Alberto; Luppi, Eleonora; Munerato, Mauro; Santoro, Valentina; Tomassetti, Luca; D., Stoker; O., Bezshyyko; G., Dolinska; N., Arnaud; C., Beigbeder; F., Bogard; D., Breton; L., Burmistrov; D., Charlet; J., Maalmi; L., Perez; V., Puill; A., Stocchi; V., Tocut; S., Wallon; G., Wormser; D., Brown; A., Calcaterra; R., de Sangro; G., Felici; G., Finocchiaro; P., Patteri; I., Peruzzi; M., Piccolo; M., Rama; S., Fantinel; G., Maron; E., Ben Haim; G., Calderini; H., Lebbolo; G., Marchiori; R., Cenci; A., Jawahery; D. A., Roberts; D., Lindemann; P., Patel; S., Robertson; D., Swersky; P., Biassoni; M., Citterio; V., Liberali; F., Palombo; A., Stabile; S., Stracka; A., Aloisio; S., Cavaliere; G., De Nardo; A., Doria; R., Giordano; A., Ordine; S., Pardi; G., Russo; C., Sciacca; A. Y., Barniakov; M. Y., Barniakov; V. E., Blinov; V. P., Druzhinin; Golubev, V. B.; S. A., Kononov; E., Kravchenko; A. P., Onuchin; S. I., Serednyakov; Y. I., Skovpen; E. P., Solodov; M., Bellato; M., Benettoni; Corvo, Marco; A., Crescente; F., Dal Corso; C., Fanin; E., Feltresi; N., Gagliardi; M., Morandin; M., Posocco; M., Rotondo; R., Stroili; C., Andreoli; L., Gaioni; E., Pozzati; L., Ratti; V., Speziali; D., Aisa; M., Bizzarri; C., Cecchi; S., Germani; P., Lubrano; E., Manoni; A., Papi; A., Piluso; A., Rossi; M., Lebeau; C., Avanzini; G., Batignani; S., Bettarini; F., Bosi; M., Ceccanti; A., Cervelli; A., Ciampa; F., Crescioli; M., Dell’Orso; D., Fabiani; F., Forti; P., Giannetti; M., Giorgi; S., Gregucci; A., Lusiani; P., Mammini; G., Marchiori; M., Massa; E., Mazzoni; F., Morsani; N., Neri; E., Paoloni; E., Paoloni; M., Piendibene; A., Profeti; G., Rizzo; L., Sartori; J., Walsh; E., Yurtsev; D. M., Asner; J. E., Fast; R. T., Kouzes; A., Bevan; F., Gannaway; J., Mistry; C., Walker; C. A. J., Brew; R. E., Coath; J. P., Crooks; R. M., Harper; A., Lintern; A., Nichols; M., Staniztki; R., Turchetta; F. F., Wilson; V., Bocci; G., Chiodi; R., Faccini; C., Gargiulo; D., Pinci; L., Recchia; D., Ruggieri; A., Di Simone; P., Branchini; A., Passeri; F., Ruggieri; E., Spiriti; D., Aston; M., Convery; G., Dubois Felsmann; W., Dunwoodie; M., Kelsey; P., Kim; M., Kocian; D., Leith; S., Luitz; D., Macfarlane; B., Ratcliff; M., Sullivan; J., Va’Vra; W., Wisniewski; W., Yang; K., Shougaev; A., Soffer; F., Bianchi; D., Gamba; G., Giraudo; P., Mereu; G., Dalla Betta; G., Fontana; G., Soncini; M., Bomben; L., Bosisio; P., Cristaudo; G., Giacomini; D., Jugovaz; L., Lanceri; I., Rashevskaya; G., Venier; L., Vitale; R., Henderson; J. F., Caron; C., Hearty; P., Lu; R., So; P., Taras; A., Agarwal; J., Franta; J. M., Rone

Studies of QCD in e+e−→e^{+}e^{-} \to hadrons at EcmE_{cm} = 130 and 136 GeV

An analysis of the properties of hadronic final states produced in electron-positron annihilation at centre-of-mass energies of 130 and 136 GeV is presented. The measurements are based on a data sample of 5.7 pb$^{-1}$ collected in November 1995 with the Aleph detector at LEP. Inclusive charged particle distributions, jet rates and event-shape distributions are measured and the results are compared with the predictions of QCD-based models. From the measured distributions quantities are determined for which the dependence on the centre-of-mass energy can be predicted by QCD, including the mean multiplicity of charged particles, the peak position of the inclusive distribution of $\xi = -\ln x_p$ ($x_p = p/p_{\rm beam}$), and the strong coupling constant $\alpha_s$. The QCD predictions are tested by comparing with corresponding measurements at $E_{\rm cm} = 91.2$ GeV and at lower energies