A paper by the Kavli Institute for the Physics and Mathematics of the Universe
(Kavli IPMU) Director Ooguri Hirosi and Project Researcher Matthew Dodelson on
the string theoretical effects outside the black hole photon sphere has been
selected for the "Editors' Suggestion" of the journal Physical Review D. Their
paper was published on March 24, 2021.

In a quantum theory of point particles, a fundamental quantity is the
correlation function, which measures the probability for a particle to
propagate from one point to another. The correlation function develops
singularities when the two points are connected by light-like trajectories.
In a flat spacetime, there is such a unique trajectory, but when spacetime
is curved, there can be many light-like trajectories connecting two points.
This is a result of gravitational lensing, which describes the effect of
curved geometry on the propagation of light.

In the case of a black hole spacetime, there are light-like trajectories
winding around the black hole several times, resulting in a black hole
photon sphere, as seen in the recent images by the Event Horizon Telescope
(EHT) of the supermassive black hole at the center of the galaxy M87.

Released on April 10, 2019, the EHT Collaboration's images captured the
shadow of a black hole and its photon sphere, the ring of light surrounding
it. A photon sphere can occur in a region of a black hole where light
entering in a horizontal direction can be forced by gravity to travel in
various orbits. These orbits lead to singularities in the aforementioned
correlation function.

However, there are cases when the singularities generated by trajectories
winding around a black hole multiple times contradict with physical
expectations. Dodelson and Ooguri have shown that such singularities are
resolved in string theory.

In string theory, every particle is considered as a particular excited state
of a string. When the particle travels along a nearly light-like trajectory
around a black hole, the spacetime curvature leads to tidal effects, which
stretch the string.

Dodelson and Ooguri showed that, if one takes these effects into account,
the singularities disappear consistently with physical expectations. Their
result provides evidence that a consistent quantum gravity must contain
extended objects such as strings as its degrees of freedom.

Ooguri says, "Our results show how string theoretical effects are enhanced
near a black hole. Though the effects we found are not strong enough to have
an observable consequence on ETH's black hole image, further research may
show us a way to test string theory using black holes."

## Reference:

Matthew Dodelson, Hirosi Ooguri. Singularities of thermal correlators at
strong coupling. Physical Review D, 2021; 103 (6) DOI:
10.1103/PhysRevD.103.066018