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| Contribution to a conference proceedings/Internal Report | PUBDB-2015-05588 |
; ;
2014
Deutsches Elektronen-Synchrotron, DESY
Hamburg
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Please use a persistent id in citations: doi:10.3204/DESY-PROC-2014-04/9
Report No.: DESY-PROC-2014-04
Abstract: The existence of a photon-like massive particle, the $\gamma'$ or dark photon, is postulated inseveral extensions of the Standard Model. Such a particle could indeed help to explain the puzzlingbehavior of the observed cosmic-ray positron fraction as well as to solve the so far unexplained deviationbetween the measured and calculated values of the muon $g-2$ anomaly. The dark photon, unlike itsconventional counterpart, would have mass and would be detectable via its mixing with the latter.We present a search for the e$^+$e$^-$ decay of such a hypothetical dark photon, also named $U$~boson, in inclusive dielectron spectra measured with HADES in the p (3.5 GeV) + p, Nb reactions, as well asin the Ar (1.756 GeV/u) + KCl reaction. A new upper limit on the kinetic mixing parametersquared ($\epsilon^2$) at 90\% CL has been obtained in the mass range $M_U$ = 0.02 -- 0.55 GeVand is compared here with the present world data set. For masses 0.03 -- 0.1 GeV, the limit has beenlowered with respect to previous results, allowing to exclude a large part of the parameter spacefavored by the muon $g-2$ anomaly.
Keyword(s): positron: cosmic radiation ; particle: massive ; mixing: kinetic ; photon ; magnetic moment ; anomaly ; HADES ; muon
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Book/Proceedings/Internal Report
Proceedings, 20th International Conference on Particles and Nuclei (PANIC 14)
Panic2014, Panic2014, HamburgHamburg, Germany, 25 Aug 2014 - 29 Aug 2014
Hamburg : Deutsches Elektronen-Synchrotron, DESY 1-754 (2014) [10.3204/DESY-PROC-2014-04]
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