The Dispersion Relation of Massive Photons in Plasma: A Comment on “Bounding the Photon Mass with Ultrawide Bandwidth Pulsar Timing Data and Dedispersed Pulses of Fast Radio Bursts”
{"title":"The Dispersion Relation of Massive Photons in Plasma: A Comment on “Bounding the Photon Mass with Ultrawide Bandwidth Pulsar Timing Data and Dedispersed Pulses of Fast Radio Bursts”","authors":"Bao Wang, Jun-Jie Wei","doi":"10.3847/2515-5172/ad7676","DOIUrl":null,"url":null,"abstract":"The dispersion measures of fast radio bursts have been identified as a powerful tool for testing the zero-mass hypothesis of the photon. The classical approach treats the massive photon-induced and plasma-induced time delays as two separate phenomena. Recently, Y.-B. Wang et al. suggested that the joint influence of the nonzero photon mass and plasma effects should be considered, and proposed a revised time delay for massive photons propagating in a plasma medium, denoted as <inline-formula>\n<tex-math>\n<?CDATA ${\\rm{\\Delta }}{t}_{{m}_{\\gamma }}^{{\\prime} }\\propto {\\nu }^{-4}$?>\n</tex-math>\n<mml:math overflow=\"scroll\"><mml:mi mathvariant=\"normal\">Δ</mml:mi><mml:msubsup><mml:mrow><mml:mi>t</mml:mi></mml:mrow><mml:mrow><mml:msub><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi>γ</mml:mi></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:mo accent=\"false\">′</mml:mo></mml:mrow></mml:msubsup><mml:mo>∝</mml:mo><mml:msup><mml:mrow><mml:mi>ν</mml:mi></mml:mrow><mml:mrow><mml:mo>−</mml:mo><mml:mn>4</mml:mn></mml:mrow></mml:msup></mml:math>\n<inline-graphic xlink:href=\"rnaasad7676ieqn1.gif\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula>, which departures from the classical dispersion relation (∝<italic toggle=\"yes\">ν</italic>\n<sup>−2</sup>). Here we discuss the derivation presented by Y.-B. Wang et al. and show that the classical dispersion relation remains valid based on Proca equations.","PeriodicalId":74684,"journal":{"name":"Research notes of the AAS","volume":"10 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Research notes of the AAS","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.3847/2515-5172/ad7676","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
The dispersion measures of fast radio bursts have been identified as a powerful tool for testing the zero-mass hypothesis of the photon. The classical approach treats the massive photon-induced and plasma-induced time delays as two separate phenomena. Recently, Y.-B. Wang et al. suggested that the joint influence of the nonzero photon mass and plasma effects should be considered, and proposed a revised time delay for massive photons propagating in a plasma medium, denoted as Δtmγ′∝ν−4, which departures from the classical dispersion relation (∝ν−2). Here we discuss the derivation presented by Y.-B. Wang et al. and show that the classical dispersion relation remains valid based on Proca equations.
快速射电暴的频散测量被认为是检验光子零质量假说的有力工具。经典方法将大质量光子诱导的时间延迟和等离子体诱导的时间延迟视为两种不同的现象。最近,Y.-B. Wang 等人提出了联合时间延迟的观点。Wang等人提出应考虑非零光子质量和等离子体效应的共同影响,并提出了大质量光子在等离子体介质中传播的修正时间延迟,表示为Δtmγ′∝ν-4,它偏离了经典色散关系(∝ν-2)。在此,我们讨论了 Y.-B. Wang 等人提出的推导,并证明Δmγ′∝ν-4 与经典色散关系(∝ν-2)相背离。王等人的推导,并证明基于普罗卡方程的经典色散关系仍然有效。