Synopsis: Testing General Relativity in a Black Hole’s Shadow

Deviations in the shadow of our Galaxy’s supermassive black hole could reveal violations of general relativity.
Synopsis figure
T. Johannsen et al., Phys. Rev. Lett. (2016)

The Event Horizon Telescope (EHT), a planet-wide network of radio telescopes, is compiling the first direct image of the giant black hole in the center of our Galaxy. The trapping of light by the hole will produce a dark shadow surrounded by a bright circular ring. A new analysis shows that the EHT could potentially detect small deviations in the shadow size, which are predicted by alternative theories of gravity.

Like most galaxies, our Milky Way has a supermassive black hole, called Sagittarius A* (Sgr A*). Observations of stars orbiting Sgr A* have provided estimates of its mass (about 4 million solar masses) and its distance from us (roughly 27,000 light years). The radius of the black hole, defined by its event horizon, is just 17 times that of the Sun. To image this compact object, astronomers formed the EHT project, which performs interferometry on data from several radio telescopes from around the globe. The group expects to have the first snapshot of Sgr A* in the next few years.

According to general relativity, the warping of space around Sgr A* creates a shadow with an apparent radius of exactly 50 microarcseconds. By contrast, many alternative gravity theories predict a larger or smaller shadow. Tim Johannsen from the Perimeter Institute for Theoretical Physics, Canada, and colleagues analyzed a previously constructed simulation of EHT data for Sgr A*. They first showed that the EHT will dramatically reduce the uncertainties in the mass and distance measurements. They also describe in detail how the EHT will test general relativity by measuring certain spacetime deviation parameters that have nonzero values in alternative gravity theories.

This research is published in Physical Review Letters.

–Michael Schirber


Announcements

More Announcements »

Subject Areas

GravitationAstrophysics

Previous Synopsis

Quantum Information

All-Around Single-Photon Source

Read More »

Next Synopsis

Mechanics

Non-Euclidean Spring

Read More »

Related Articles

Synopsis: Skydiving Spins
Gravitation

Synopsis: Skydiving Spins

Atom interferometry shows that the free-fall acceleration of rubidium atoms of opposite spin orientation is the same to within 1 part in 10 million. Read More »

Synopsis: Solar Cycle Affects Cosmic Ray Positrons
Astrophysics

Synopsis: Solar Cycle Affects Cosmic Ray Positrons

Discrepancies in the positron content of cosmic rays measured at different times are explained by the periodic reversal of the solar magnetic field’s direction. Read More »

Focus: LIGO Bags Another Black Hole Merger
Astrophysics

Focus: LIGO Bags Another Black Hole Merger

LIGO has detected a second burst of gravitational waves from merging black holes, suggesting that such detections will soon become routine and part of a new kind of astronomy. Read More »

More Articles