2011
DOI: 10.1140/epjc/s10052-011-1611-8
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Global study of electron–quark unparticle interactions

Abstract: We perform a global fit on parity-conserving electron-quark interactions via spin-1 unparticle exchange. Besides the peculiar features of unparticle exchange due to non-integral values for the scaling dimension d U and a non-trivial phase factor exp(−id U π) associated with a time-like unparticle propagator, the energy dependence of the unparticle contributions in the scattering amplitudes are also taken into account. The high energy data sets taken into consideration in our analysis are from (1) deep inelasti… Show more

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Cited by 10 publications
(23 citation statements)
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References 28 publications
(51 reference statements)
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“…Where such vacuum electromagnetic shocks and accompanying harmonic generation might play a role, is in the evolution of X-ray pulsars and strongly-magnetised neutron stars or "magnetars" [91][92][93]. Photons are emitted from the surface of such objects and propagate through magnetic fields of strength up to and beyond E cr (in the system of units we use, B cr = E cr ), in plasmas of around 0.1-10 cm in depth [94].…”
Section: Measurabilitymentioning
confidence: 99%
“…Where such vacuum electromagnetic shocks and accompanying harmonic generation might play a role, is in the evolution of X-ray pulsars and strongly-magnetised neutron stars or "magnetars" [91][92][93]. Photons are emitted from the surface of such objects and propagate through magnetic fields of strength up to and beyond E cr (in the system of units we use, B cr = E cr ), in plasmas of around 0.1-10 cm in depth [94].…”
Section: Measurabilitymentioning
confidence: 99%
“…In our phenomenological analysis, as well as in those performed in Refs. [12,16,17], leptons and quarks contained in the H and D fields are neglected and assumed to be too heavy to contribute to Z ′ phenomenology. We are nevertheless aware that this is a quite strong assumption and that in forthcoming BSM investigations one may well assume that such exotics leptons and quarks (sleptons and squarks) are lighter than the Z ′ and therefore they can contribute to Z ′ decays.…”
Section: U(1) ′ Models and Chargesmentioning
confidence: 99%
“…[6] and improves Refs. [7,8] by consistently including the so-called D-term correction, due to the extra U (1) ′ group, to the sfermion masses. The U (1) ′ groups result from the breaking of a rank-6 GUT group E 6 → SO(10) × U(1) …”
Section: Introductionmentioning
confidence: 99%