2012
DOI: 10.1007/jhep02(2012)134
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Price for environmental neutrino-superluminality

Abstract: Abstract:We ask whether the recent OPERA results on neutrino superluminality could be an environmental effect characteristic of the local neighborhood of our planet, without the need of violation of the Poincaré-invariance at a fundamental level. We show, that model-indepenently, such a possibility implies the existence of new gravitational degrees of freedom. Namely, this explanation requires the existence of a new spin-2 field of a planetary Compton wave-length that is coupled to neutrinos and the rest of th… Show more

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Cited by 48 publications
(67 citation statements)
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References 21 publications
(41 reference statements)
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“…For earlier studies on superluminal motions of neutrinos in various frameworks, see, e.g., [10,11,12,13,14,15,16]. Dvali and Vikman [17] wondered if the OPERA superluminal phenomenology could be an environmental effect characteristic of the local neighborhood of the Earth, without the need of violation of the Poincaré invariance at a fundamental level. Such a scenario, at an effective field theory level, yields naturally an inevitable appearance of a testable long-range fifth force of gravitational type.…”
Section: Introductionmentioning
confidence: 99%
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“…For earlier studies on superluminal motions of neutrinos in various frameworks, see, e.g., [10,11,12,13,14,15,16]. Dvali and Vikman [17] wondered if the OPERA superluminal phenomenology could be an environmental effect characteristic of the local neighborhood of the Earth, without the need of violation of the Poincaré invariance at a fundamental level. Such a scenario, at an effective field theory level, yields naturally an inevitable appearance of a testable long-range fifth force of gravitational type.…”
Section: Introductionmentioning
confidence: 99%
“…= c 5 8πG = 2.43 × 10 18 GeV is the energy equivalent of the reduced Planck's mass, where is the reduced Planck constant, c is the speed of light in vacuum and G is the Newtonian constant of gravitation, and the scale M * sets the strength of the coupling of the putative new massive spin-2 degree of freedom to the neutrino [17]. For other investigations involving various aspects of gravitation, astrophysics and cosmology, see, e.g., [19,20,21,22,23,24,25,26,27,28,29,30,31].…”
Section: Introductionmentioning
confidence: 99%
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“…From the consistent models proposed, most attempted to accommodate the result by parametrizing appropriately the neutrino couplings in the SM. The two extra alternatives proposed included a new massive graviton interaction, [86] and a new scalar interaction [87].…”
Section: Resultsmentioning
confidence: 99%
“…This is achieved thanks to screening features such as the Vainshtein mechanism for theories with higher order derivative self interactions [2], or the chameleon [3], symmetron [4] or Damour-Polyakov properties [5] for theories with non-linear effective potentials in the presence of pressure-less matter. Recently and after the claim of super-luminal propagation of neutrinos by the OPERA experiment [6], it has been suggested that fermions may travel faster than the speed of light in dense environments where the presence of matter offers a breaking of Lorentz invariance [7]. This was further pursued in [8][9][10] and then in [11] where Galileons were used to describe the OPERA claims although failing to respect the tight bounds on the deviation of the electron speed from the speed of light.…”
Section: Pacs Numbersmentioning
confidence: 99%