2020
DOI: 10.1016/j.scib.2019.11.024
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Light speed variation from active galactic nuclei

Abstract: Recent studies on the high-energy photons from gamma-ray bursts (GRBs) suggested a light speed variation v(E) = c(1 − E/ELV) with ELV = 3.6 × 10 17 GeV. We check this speed variation from previous observations on light curves of three active galactic nuclei (AGNs), namely Markarian 421 (Mrk 421), Markarian 501 (Mrk 501) and PKS 2155-304. We show that several phenomena related to the light curves of these AGNs can serve as the supports for the light speed variation determined from GRBs.

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Cited by 21 publications
(14 citation statements)
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“…which is close to the Planck scale E Pl ≃ 1.22 × 10 19 GeV. It is worth noting that such a LV scale ( 7) is consistent with various constraints from high-energy γ-ray observations of pulsars [19], AGNs [21,22,23] as well as GRBs [24,25,26,27,28], and it is also compatible with the strongest robust limit to date from a recent study [29] on 8 Fermi-LAT GRBs. We should mention that there can be severer bounds to E LV from other time-delay studies (see, e.g., Ref.…”
supporting
confidence: 86%
“…which is close to the Planck scale E Pl ≃ 1.22 × 10 19 GeV. It is worth noting that such a LV scale ( 7) is consistent with various constraints from high-energy γ-ray observations of pulsars [19], AGNs [21,22,23] as well as GRBs [24,25,26,27,28], and it is also compatible with the strongest robust limit to date from a recent study [29] on 8 Fermi-LAT GRBs. We should mention that there can be severer bounds to E LV from other time-delay studies (see, e.g., Ref.…”
supporting
confidence: 86%
“…[53], time delays between two light curves of different energy bands of PKS 2155-304 were used to give a lower bound of E LIV > 7.2 × 10 17 GeV. However a latest work [55] points out a novel way to understand the delays which can be considered as a signal for the light speed variation with E LIV ≃ 3.6 × 10 17 GeV, i.e., Eq. (21).…”
Section: Velocity Dispersion Of Light In the D-particle Quantumgravitational Foam Mediummentioning
confidence: 99%
“…In fact, intensive studies have been performed on the n = 3 case of Eq. ( 7) based on time of light flight observations of high energy photons from GRBs [15,[26][27][28][29][30][31][32][33] and active galactic nuclei (AGNs) [34]. These researches suggest ξ = E −1 LV , where E LV = 3.6 × 10 17 GeV, see, e.g., Ref.…”
mentioning
confidence: 99%