'Naked singularity' detection now easier? Indian scientists find new ways!

Wikipedia defines naked singularity as "a gravitational singularity without an event horizon."

By Zee Media Bureau | Updated: Apr 21, 2017, 15:28 PM IST
'Naked singularity' detection now easier? Indian scientists find new ways!
Image courtesy: YouTube (Representational image)

New Delhi: A significant discovery has led a team of Indian scientists to come across novel means of detecting the most extreme object in the universe – a bare or naked 'singularity'.

Wikipedia defines naked singularity as “a gravitational singularity without an event horizon. In a black hole, the singularity is completely enclosed by a boundary known as the event horizon, inside which the gravitational force of the singularity is so strong that light cannot escape. Hence, objects inside the event horizon—including the singularity itself—cannot be directly observed. A naked singularity, by contrast, is observable from the outside.”

This means that, when the fuel of a very massive star is spent, it collapses owing to its own gravitational pull and eventually becomes a very small region of arbitrarily high matter density, that is a "Singularity" where the usual laws of physics may breakdown.

However, if this "singularity" is hidden within an event horizon, which is an invisible closed surface from which nothing, not even light, can escape, then we call this object a black hole.

In such a case, we cannot see the "singularity" and we do not need to bother about its effects.

But what if the event horizon does not form?

To address this, Dr Chandrachur Chakraborty, Prashant Kocherlakota and Professor Sudip Bhattacharyya and Professor Pankaj Joshi -- in collaboration with a Polish team comprising Dr Mandar Patil and Professor Andrzej Krolak -- have shown that the precession frequency of a gyroscope orbiting a black hole or a naked "singularity" is sensitive to the presence of an event horizon.

Scientists from the Tata Institute of Fundamental Research (TIFR) in Mumbai responsible for the findings, have recently argued that the rate at which a gyroscope precesses (the precession frequency), when placed around a rotating black hole or a naked "singularity", could be used to identify this rotating object.

A gyroscope circling and approaching the event horizon of a black hole from any direction behaves increasingly 'wildly,' that is, it precesses increasingly faster, without a bound.

But, in the case of a naked "singularity", the precession frequency becomes arbitrarily large only in the equatorial plane, but being regular in all other planes.

The TIFR team has also found that the precession of orbits of matter falling into a rotating black hole or a naked "singularity" can be used to distinguish these exotic objects.

"This is because the orbital plane precession frequency increases as the matter approaches a rotating black hole, but this frequency can decrease and even become zero for a rotating naked singularity," the team noted in a paper appeared in the journal Physical Review D.

The finding could be used to distinguish a naked "singularity" from a black hole in reality, because the precession frequencies could be measured in X-ray wavelengths, as the infalling matter radiates X-rays.

(With IANS inputs)