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The frequency-dependent time delays in fast radio bursts (FRBs) can be used to constrain the photon mass, if the FRB redshifts are known, but the similarity between the frequency dependences of dispersion due to plasma effects and a photon…

The photon mass, $m_\gamma$, can in principle be constrained using measurements of the dispersion measures (DMs) of fast radio bursts (FRBs), once the FRB redshifts are known. The DM of the repeating FRB 121102 is known to $< 1$\%, a host…

Fast radio bursts (FRBs) have been suggested as an excellent celestial laboratory for testing the zero-mass hypothesis of the photon. In this work, we use the dispersion measure (DM)--redshift measurements of 23 localized FRBs to revisit…

High Energy Astrophysical Phenomena · Physics 2023-08-30 Bao Wang , Jun-Jie Wei , Xue-Feng Wu , Martín López-Corredoira

A hypothetical photon mass, $m_\gamma$, gives an energy-dependent light speed in a Lorentz-invariant theory. Such a modification causes an additional time delay between photons of different energies when they travel through a fixed…

High Energy Physics - Phenomenology · Physics 2017-06-20 Lijing Shao , Bing Zhang

We constrain the photon mass from well-localized fast radio bursts (FRBs) using Bayes inference method. The probability distributions of dispersion measures (DM) of host galaxy and intergalactic medium are properly taken into account. The…

General Relativity and Quantum Cosmology · Physics 2023-09-21 Hai-Nan Lin , Li Tang , Rui Zou

The assumption that photons are massless is a foundational postulate of modern physics, yet it remains subject to experimental verification. Fast radio bursts (FRBs), with their cosmological distances and precisely measured dispersion,…

Cosmology and Nongalactic Astrophysics · Physics 2026-01-26 Yuchen Zhang , Yang Liu , Hongwei Yu , Puxun Wu

Photon is the fundamental quantum of electromagnetic fields, whose mass, $m_{\gamma}$, should be strictly zero in Maxwell's theory. But not all theories adopt this hypothesis. If the rest mass of the photon is not zero, there will be an…

High Energy Astrophysical Phenomena · Physics 2021-09-01 Huimei Wang , Xueli Miao , Lijing Shao

A hypothetical photon mass, $m_{\gamma}$, can produce a frequency-dependent vacuum dispersion of light, which leads to an additional time delay between photons with different frequencies when they propagate through a fixed distance. The…

Cosmology and Nongalactic Astrophysics · Physics 2024-04-29 Jing-Yu Ran , Bao Wang , Jun-Jie Wei

Fast radio bursts (FRBs) offer a powerful probe of the ionized Universe through their dispersion measures (DM). While a significant fraction of the DM arises from the intergalactic medium (IGM), the contributions from the host galaxy and…

Cosmology and Nongalactic Astrophysics · Physics 2026-03-13 Gunalan Muthusami , Gopal Kashyap

The photon zero-mass hypothesis has been investigated for a long time using the frequency-dependent time delays of radio emissions from astrophysical sources. However, the search for a rest mass of the photon has been hindered by the…

High Energy Astrophysical Phenomena · Physics 2018-08-08 Jun-Jie Wei , Xue-Feng Wu

Exploring the concept of a massive photon has been an important area in astronomy and physics. If photons have mass, their propagation in nonvacuum space would be affected by both the nonzero mass $m_{\gamma}$ and the presence of a plasma…

High Energy Astrophysical Phenomena · Physics 2024-04-04 Yu-Bin Wang , Xia Zhou , Abdusattar Kurban , Fa-Yin Wang

Fast radio bursts (FRBs) are radio bursts characterized by millisecond durations, high Galactic latitude positions, and high dispersion measures. Very recently, the cosmological origin of FRB 150418 has been confirmed by \cite{kea16}, and…

High Energy Astrophysical Phenomena · Physics 2016-05-04 Xue-Feng Wu , Song-Bo Zhang , He Gao , Jun-Jie Wei , Yuan-Chuan Zou , Wei-Hua Lei , Bing Zhang , Zi-Gao Dai , Peter Mészáros

Electromagnetic emissions from astrophysical sources at cosmological distances can be used to estimate the photon mass, $m_{\gamma}$. In this paper, we combine measurements of the dispersion measure ($\mathrm{DM}$) of fast radio bursts…

Cosmology and Nongalactic Astrophysics · Physics 2025-05-01 Thais Lemos , Rodrigo Gonçalves , Joel Carvalho , Jailson Alcaniz

A conservative constraint on the rest mass of the photon can be estimated under the assumption that the frequency dependence of dispersion from astronomical sources is mainly contributed by the nonzero photon mass effect. Photon mass limits…

High Energy Astrophysical Phenomena · Physics 2017-03-08 Jun-Jie Wei , Er-Kang Zhang , Song-Bo Zhang , Xue-Feng Wu

The gravitational time delays of macro-lenses can be used to constrain the rest mass of the photon with high accuracy. Assuming a point-mass $+$ external shear lens model, we prove that an upper limit of the photon mass can be derived…

High Energy Astrophysical Phenomena · Physics 2025-01-28 Chen-Ming Chang , Jun-Jie Wei , Ke-Lai Meng , Song-Bo Zhang , Hao-Xuan Gao , Jin-Jun Geng , Xue-Feng Wu

Radio signals propagating through inhomogeneous plasma media deviate from their original paths, producing frequency-dependent magnification effects. In this paper, after reviewing the classical plasma-lensing theory, we have found a…

High Energy Astrophysical Phenomena · Physics 2025-09-26 Yu-Bin Wang , Xia Zhou , Abdusattar Kurban

We summarize our understanding of millisecond radio bursts from an extragalactic population of sources. FRBs occur at an extraordinary rate, thousands per day over the entire sky with radiation energy densities at the source about ten…

High Energy Astrophysical Phenomena · Physics 2019-09-11 James M. Cordes , Shami Chatterjee

Tight limits on the photon mass have been set through analyzing the arrival time differences of photons with different frequencies originating from the same astrophysical source. However, all these constraints have relied on using the…

High Energy Astrophysical Phenomena · Physics 2023-01-18 Chen-Ming Chang , Jun-Jie Wei , Song-Bo Zhang , Xue-Feng Wu

Fast Radio Bursts (FRBs) are millisecond transient radio events with a high energy. By identifying the origin of the \textbf{burst}, it is possible to measure the redshift of the host galaxy, which can be used to constrain cosmological and…

Cosmology and Nongalactic Astrophysics · Physics 2024-02-27 Thais Lemos , Rodrigo S. Gonçalves , Joel C. Carvalho , Jailson S. Alcaniz

Fast radio bursts (FRBs) have excessive dispersion measures (DMs) and an all-sky distribution, which point toward an extragalactic or even a cosmological origin. We develop a method to extract the mean host galaxy DM ($\left\langle{\rm…

High Energy Astrophysical Phenomena · Physics 2017-04-26 Yuan-Pei Yang , Rui Luo , Zhuo Li , Bing Zhang
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