Search for dark photons produced in 13 TeV $pp$ collisions

Searches are performed for both promptlike and long-lived dark photons, A 0 , produced in proton-proton collisions at a center-of-mass energy of 13 TeV, using A 0 → μ þ μ − decays and a data sample corresponding to an integrated luminosity of 1 . 6 fb − 1 collected with the LHCb detector. The prompt...

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Hauptverfasser: Adinolfi, M, Akar, S, Alessio, F, Anderlini, L, Baalouch, M, Badalov, A, Beaucourt, L, Belloli, N, Bertholet, E, Blusk, S, Bowcock, TJV, Braun, S, Buytaert, J, Carboni, G, Ciambrone, P, Vidal, XC, Clarke, PEL, Paula, LD, Dean, CT, Dziewiecki, M, Fazzini, D, Declara, PF, Fiorini, M, Fleuret, F, Frank, M, Gizdov, K, Graugés, E, Graverini, E, Grillo, L, Guz, Y, Han, X, He, J, Heß, M, Humair, T, Hutchcroft, D, Jacobsson, R, Jalocha, J, Johnson, D, Khanji, B, Klaver, S, Kosmyntseva, A, Kruse, F, Kuonen, AK, Lai, A, Li, Y, Luo, H, Machefert, F, Mackowiak, P, Maltsev, T, Martellotti, G, Massafferri, A, Matev, R, Mauri, A, Meaux, C, Millard, E, Minzoni, L, Morello, MJ, Müller, V, Needham, M, Neubert, S, Neufeld, N, Nikodem, T, O'Hanlon, DP, Onderwater, CJG, Owen, P, Patrignani, C, Pearce, A, Pellegrino, A, Petrolini, A, Playfer, S, Poslavskii, S, Price, E, Ricciardi, S, Rinnert, K, Robbe, P, Sadykhov, E, Guimaraes, VS, Santacesaria, R, Santovetti, E, Sarpis, G, Sepulveda, ES, Serrano, J, Sokoloff, MD, Sun, J, Tobin, M, Tolk, S, Tonelli, D, Tully, A, Valenti, G, Velthuis, JJ, Vernet, M, Viemann, H, Sierra, CV, Ward, DR, Wilkinson, G, Winn, M, Witek, M, Wormser, G, Xu, Z, Yao, Y
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Zusammenfassung:Searches are performed for both promptlike and long-lived dark photons, A 0 , produced in proton-proton collisions at a center-of-mass energy of 13 TeV, using A 0 → μ þ μ − decays and a data sample corresponding to an integrated luminosity of 1 . 6 fb − 1 collected with the LHCb detector. The promptlike A 0 search covers the mass range from near the dimuon threshold up to 70 GeV, while the long-lived A 0 search is restricted to the low-mass region 214
DOI:10.1103/PhysRevLett.120.061801