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• W3103258514 startingPage "23" @default.
• W3103258514 abstract "Pulsars are magnetized rotating compact objects. They spin down due to magnetic dipole radiation and wind emission. If photon has a nonzero mass, the spin down rate would be smaller than the zero mass case. We show that an upper limit of the photon mass, i.e. $m_gammalesssim h/Pc^2$, may be placed if a pulsar with period $P$ is observed to spin down. Recently, a white dwarf (WD) --- M dwarf binary, AR Scorpii was discovered to emit pulsed broadband emission with pulses. The spin-down luminosity of the WD can comfortably power the non-thermal radiation from the system. Applying our results to the WD pulsar with $P=117~rm{s}$, we obtain a stringent upper limit of the photon mass between $m_gamma<6.3times10^{-50}~rm{g}$ assuming a vacuum dipole spindown, and $m_gamma<9.6times10^{-50}~rm{g}$ assuming a spindown due to a fully developed pulsar wind." @default.
• W3103258514 created "2020-11-23" @default.
• W3103258514 creator A5015654535 @default.
• W3103258514 creator A5045473616 @default.
• W3103258514 date "2017-06-08" @default.
• W3103258514 modified "2023-09-23" @default.
• W3103258514 title "Tight Constraint on Photon Mass from Pulsar Spindown" @default.
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• W3103258514 doi "https://doi.org/10.3847/1538-4357/aa74de" @default.
• W3103258514 hasPublicationYear "2017" @default.
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