2021
DOI: 10.1103/physrevd.104.063012
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Ultrahigh-energy photons from LHAASO as probes of Lorentz symmetry violations

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Cited by 24 publications
(34 citation statements)
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“…On the other hand, astroparticle experiments by means of ultra high energy (UHE) photons coming from gamma ray burst (GRB), are exploring the Universe on the largest energy scales observed so far. Particularly, the LHAASO experiment has detected on the Earth's surface, gamma rays at the PeV energy scale [7][8][9][10][11][12]. These detections are not in agreement with those models where the photon relation dispersion is of the form ω 2 ∝ k 2 .…”
Section: Introductionmentioning
confidence: 82%
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“…On the other hand, astroparticle experiments by means of ultra high energy (UHE) photons coming from gamma ray burst (GRB), are exploring the Universe on the largest energy scales observed so far. Particularly, the LHAASO experiment has detected on the Earth's surface, gamma rays at the PeV energy scale [7][8][9][10][11][12]. These detections are not in agreement with those models where the photon relation dispersion is of the form ω 2 ∝ k 2 .…”
Section: Introductionmentioning
confidence: 82%
“…On the other hand, it can be shown from the constraint (2) and the T+L decomposition, that the longitudinal part of the momentum E Li of the gauge sector is zero [39,40]. Now, to infer the behavior of the remaining canonical variables ı.e., g ij and N , we need to use the second class constraints (7) and (8) together with the previous estimation on the components of the momentum π ij . The suitable combination 2H p + H N of the constraints ( 7) and ( 8) leads to ∆N B…”
Section: B Constraints Solutionmentioning
confidence: 99%
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“…Among these proposals, a prominent role is played by the those that predict a violation or deformation of the special relativistic principles (referred as LIV and DSR scenarios, respectively) in the regime in which → 0 and G → 0, but that preserves the Planck energy scale E P = c 5 /G ≈ 1.22 × 10 19 GeV. The phenomenological opportunities of this approach range among several areas, for instance threshold effects in particle interactions [6][7][8], time delays in the arrivals of relativistic particles with different energies due to modified dispersion relations (MDRs) [9][10][11][12][13][14][15]), gravitational lensing observations [16,17], violation of CPT symmetry [18,19], etc (we refer the reader to Refs. [4,5,20] for reviews in modern searches of these effects).…”
Section: Introductionmentioning
confidence: 99%