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Galactic Shapiro delay to the Crab pulsar and limit on weak equivalence principle violation

dc.contributor.authorDesai, Shantanu
dc.contributor.authorKahya, Emre
dc.date.accessioned2026-01-25T02:49:18Z
dc.date.issued2018-01-30
dc.description.abstractWe calculate the total galactic Shapiro delay to the Crab pulsar by including the contributions from the dark matter as well as baryonic matter along the line of sight. The total delay due to dark matter potential is about 3.4 days. For baryonic matter, we included the contributions from both the bulge and the disk, which are approximately 0.12 and 0.32 days respectively. The total delay from all the matter distribution is therefore 3.84 days. We also calculate the limit on violations of Einstein's equivalence principle by using observations of "nano-shot" giant pulses from the Crab pulsar with time-delay $<0.4$~ns as well as using time differences between radio and optical photons observed from this pulsar. Using the former, we obtain a limit on violation of Einstein's equivalence principle in terms of the PPN parameter $����< 2.41\times 10^{-15}$. From the time-difference between simultaneous optical and radio observations, we get $����< 1.54\times 10^{-9}$. We also point out differences in our calculation of Shapiro delay and that from two recent papers (arXiv:1612.00717 and arXiv:1608.07657), which used the same observations to obtain a corresponding limit on $����$.
dc.description.abstract4 pages, 1 figure. Accepted for publication in Eur. Phys. Journal C
dc.description.urihttps://doi.org/10.1140/epjc/s10052-018-5571-0
dc.description.urihttps://link.springer.com/content/pdf/10.1140%2Fepjc%2Fs10052-018-5571-0.pdf
dc.description.urihttps://dx.doi.org/10.48550/arxiv.1612.02532
dc.description.urihttp://arxiv.org/abs/1612.02532
dc.description.urihttps://doaj.org/article/308ffd99484448008817ab0aaabe65a9
dc.description.urihttps://dx.doi.org/10.1140/epjc/s10052-018-5571-0
dc.description.urihttps://aperta.ulakbim.gov.tr/record/106997
dc.description.urihttps://doi.org/https://doi.org/10.1140/epjc/s10052-018-5571-0
dc.identifier.doi10.1140/epjc/s10052-018-5571-0
dc.identifier.eissn1434-6052
dc.identifier.issn1434-6044
dc.identifier.openairedoi_dedup___::50f25a16e28e1457369a500b0cb1b6ac
dc.identifier.orcid0000-0002-0466-3288
dc.identifier.urihttps://hdl.handle.net/11527/43240
dc.identifier.volume78
dc.language.isoeng
dc.publisherSpringer Science and Business Media LLC
dc.relation.ispartofThe European Physical Journal C
dc.rightsOPEN
dc.subjectQB460-466
dc.subjectHigh Energy Astrophysical Phenomena (astro-ph.HE)
dc.subjectNuclear and particle physics. Atomic energy. Radioactivity
dc.subjectFOS: Physical sciences
dc.subjectQC770-798
dc.subjectAstrophysics
dc.subjectAstrophysics - High Energy Astrophysical Phenomena
dc.titleGalactic Shapiro delay to the Crab pulsar and limit on weak equivalence principle violation
dc.typeArticle
dspace.entity.typePublication

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