Sensitivity of the SHiP experiment to dark photons decaying to a pair of charged particles
C. Ahdida, Atakan Tugberk Akmete, R. Albanese, A. Alexandrov, A. Anokhina, S. Aoki, G. Arduini, E. Atkin, N. Azorskiy, J. J. Back, A. Bagulya, F. Baaltasar dos Santos, A. Baranov, F. Bardou, Gareth J. Barker, M. Battistin, J. Bauche, A. Bay, V. Bayliss, G. Bencivenni, A. Berdnikov, Y. Berdnikov, M. Bertani, C. Betancourt, Ia. Bezshyiko, O. Bezshyyko, D. Bick, S. Bieschke, A. Blanco, J. Boehm, M. Bogomilov, I. Boiarska, Kyrylo Bondarenko, W. Bonivento, J. Borburgh, Alexey Boyarsky, R. Brenner, D. Breton, V. Büscher, A. Buonaura, S. Buontempo, S. Cadeddu, A. Calcaterra, M. Calviani, M. Campanelli, M. Casolino, N. Charitonidis, P. Chau, J. Chauveau, A. Chepurnov, M. Chernyavskiy, Ki-Young Choi, А. Г. Чумаков, P. Ciambrone, V. Cicero, L. Congedo, Karel Cornelis, M. Cristinziani, A. Crupano, G. M. Dallavalle, A. Dätwyler, N. D’Ambrosio, G. D’Appollonio, R. de Asmundis, J. de Carvalho Saraiva, G. De Lellis, Matteo Magistris, A. De Roeck, M. de Serio, D. De Simone, L. Dedenko, Pavel Dergachev, A. Di Crescenzo, L. Di Giulio, N. Di Marco, Claudio Dib, H. Dijkstra, В. В. Дмитренко, L. A. Dougherty, A. Dolmatov, D. Domenici, S.V. Donskov, V. Drohan, A. Dubreuil, O. Durhan, M. Ehlert, E. Elikkaya, T. Enik, A. Etenko, F. Fabbri, O. L. Fedin, F. Fedotovs, G. Felici, Martina Ferrillo, M. Ferro-Luzzi, K. Filippov, R. A. Fini, P. Fonte, C. Franco, M. Fraser
Abstract
Abstract Dark photons are hypothetical massive vector particles that could mix with ordinary photons. The simplest theoretical model is fully characterised by only two parameters: the mass of the dark photon m $$_{\gamma ^{\mathrm {D}}}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mrow/> <mml:msup> <mml:mi>γ</mml:mi> <mml:mi>D</mml:mi> </mml:msup> </mml:msub> </mml:math> and its mixing parameter with the photon, $$\varepsilon $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>ε</mml:mi> </mml:math> . The sensitivity of the SHiP detector is reviewed for dark photons in the mass range between 0.002 and 10 GeV. Different production mechanisms are simulated, with the dark photons decaying to pairs of visible fermions, including both leptons and quarks. Exclusion contours are presented and compared with those of past experiments. The SHiP detector is expected to have a unique sensitivity for m $$_{\gamma ^{\mathrm {D}}}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mrow/> <mml:msup> <mml:mi>γ</mml:mi> <mml:mi>D</mml:mi> </mml:msup> </mml:msub> </mml:math> ranging between 0.8 and 3.3 $$^{+0.2}_{-0.5}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msubsup> <mml:mrow/> <mml:mrow> <mml:mo>-</mml:mo> <mml:mn>0.5</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>0.2</mml:mn> </mml:mrow> </mml:msubsup> </mml:math> GeV, and $$\varepsilon ^2$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msup> <mml:mi>ε</mml:mi> <mml:mn>2</mml:mn> </mml:msup> </mml:math> ranging between $$10^{-11}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msup> <mml:mn>10</mml:mn> <mml:mrow> <mml:mo>-</mml:mo> <mml:mn>11</mml:mn> </mml:mrow> </mml:msup> </mml:math> and $$10^{-17}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msup> <mml:mn>10</mml:mn> <mml:mrow> <mml:mo>-</mml:mo> <mml:mn>17</mml:mn> </mml:mrow> </mml:msup> </mml:math> .