Synopsis: Black Holes Weigh the Possibility of a Massive Photon

New calculations of hypothetical “black hole bombs” set an upper limit on the possible mass of the photon and on the existence of certain dark matter candidates.

Black holes don’t usually get pushed around, but a very lightweight particle can theoretically stop a rotating black hole by setting off a so-called “black-hole bomb.” New calculations reported in Physical Review Letters show that photons, or photonlike particles, could be considered bomb-making material if they have a mass. A massive photon is not theoretically ruled out, but it would have implications for the dispersion of light and the existence of magnetic monopoles. However, the mere existence of spinning (unbombed) black holes constrains this possibility, thus allowing the authors to put the most stringent limit yet on the mass of the photon.

Falling into a black hole means curtains for most things. But physicists have shown that a hypothetical spin-zero particle—called a scalar boson—could quantum-mechanically bind to a rotating black hole if the particle’s Compton wavelength (which is inversely proportional to its mass) is roughly equal to the radius of the black hole. The resulting gravitational “atom” would lead to a runaway effect, or bomb, that zaps the hole’s rotational energy in a relatively short time.

Paolo Pani, at the Technical University of Lisbon in Portugal, and his colleagues extended these investigations to massive spin-one particles, such as massive photons. The calculations in this case are extremely difficult, so the researchers studied slowly rotating black holes and then extrapolated their results to fast rotation. They found that massive spin-one particles trigger more powerful “bombs” than scalar (spin-zero) particles. The observed rotation of supermassive black holes rules out photons (as well as photonlike particles, that some theories suggest could contribute to dark matter) of mass above 4×10-20eV. – Michael Schirber


Features

More Features »

Announcements

More Announcements »

Subject Areas

Gravitation

Previous Synopsis

Interdisciplinary Physics

The Value of Circular Definitions

Read More »

Related Articles

Synopsis: Searching for Neutron Star Gravitational Waves
Astrophysics

Synopsis: Searching for Neutron Star Gravitational Waves

The first run of LIGO and Virgo’s gravitational-wave search shows no evidence of spinning asymmetric neutron stars, but recent upgrades could make the detection possible. Read More »

Viewpoint: Spinning Black Holes May Grow Hair
Gravitation

Viewpoint: Spinning Black Holes May Grow Hair

A spinning black hole may lose up to 9% of its mass by spontaneously growing “hair” in the form of excitations of a hypothetical particle field with a tiny mass. Read More »

Synopsis: LIGO’s Black Hole Got the Boot
Astrophysics

Synopsis: LIGO’s Black Hole Got the Boot

An analysis of data from LIGO’s second gravitational-wave event indicates that a supernova can impart a strong kick to the black hole it creates. Read More »

More Articles