Home

New discovery: It may be the holy grail of pulsar astronomy

: 19.01.2024

Professor of astrophysics Thomas Tauris (AAU) has, together with an international team of astronomers, identified the first known system in which a so-called millisecond pulsar probably orbits a black hole. According to Thomas Tauris, the discovery challenges the limits of the imagination and may lead to clarification of Einstein's general theory of relativity.

New discovery: It may be the holy grail of pulsar astronomy

: 19.01.2024

Professor of astrophysics Thomas Tauris (AAU) has, together with an international team of astronomers, identified the first known system in which a so-called millisecond pulsar probably orbits a black hole. According to Thomas Tauris, the discovery challenges the limits of the imagination and may lead to clarification of Einstein's general theory of relativity.

By David Graff, AAU Communication and Public Affairs. Photo: Daniëlle Futselaar

When Professor Thomas Tauris in the autumn of 2022 began to analyze the observations his colleagues at the Max Planck Institute in Bonn had obtained via the MeerKAT radio telescope, he was thrilled like a child on Christmas Eve:

"Research in the Universe continues to surprise, but this finding is something out of the ordinary – the combination of a millisecond pulsar and a mysterious compact object that is likely a black hole is probably what my pulsar colleagues have been looking most for in the last 40 to 50 years," he says.

The discovery was made in our galaxy, specifically in a star cluster (globular cluster) called NGC 1851, where the stars swarm closely and constantly influence each other.

Our ultimate hope is that we can get one step closer to unifying Einstein's general theory of relativity and quantum mechanics in our understanding of gravity.

Professor of astrophysics at Aalborg University Thomas Tauris

Chance of fundamental breakthrough

The researchers' excitement stems from the fact that the combination of a millisecond pulsar and a black hole in a binary system may provide an opportunity to test Einstein's general theory of relativity at points where the theory is not entirely clear. Hence, the door may open to clarifying one of the most important scientific theories of the 20th century.

- Our ultimate hope is that we can get one step closer to unifying Einstein's general theory of relativity and quantum mechanics in our understanding of gravity, explains Thomas Tauris. However, he stresses that it is far too early to say whether it will succeed.

In order for it to be even possible in principle to further develop the theory of relativity, the object around which the millisecond pulsar orbits in the newfound system must be a black hole. But it is not yet clarified whether this is the case.

An artist's impression of the system under the assumption that the millisecond pulsar orbits a black hole. The bright background “star” is the millisecond radio pulsar PSR J0514-4002E. The two objects are separated by 8 million kilometers and orbit each other every seven days.
Photo: Daniëlle Futselaar (artsource.nl)

Never seen before

The study of the binary system takes place through calculations of mass, orbital motion, rotation, gravity and radiation, and it has not yet been possible to determine what the object around which the millisecond pulsar orbits is. It can be either a black hole or a record high-mass neutron star.

Both types of compact objects are characterized by dense mass and the influence on its surroundings through gravity.

Furthermore, calculations have revealed that if it is a black hole, it is the lightest version of such a hole ever measured. In the case of a neutron star, it is the heaviest version ever measured.

In the coming years, researchers will try to determine which of the two phenomena they have discovered – or whether it may be something third - a hitherto unknown exotic object with a mass between that of a black hole and a neutron star.

However, one thing is certain: With this discovery, scientists have found a unique laboratory to study fundamental physics in the form of gravity and the properties of matter under the most extreme conditions in the Universe.

thumbnail

The NGC 1851E System

Watch an orbital simulation detailing a possible formation channel for the NGC 1851E system.

:

The NGC 1851E System

Watch an orbital simulation detailing a possible formation channel for the NGC 1851E system.

Video: OzGrav ARC Centre of Excellence

FACTS: Neutron stars, black holes, and the black hole mass gap

Neutron stars are ultra-dense remnants of supernova explosions, and there are limits to how massive they can be. When they have accumulated too much mass by, for example, absorbing other stars, they will collapse. What exactly they will become when they collapse is the subject of much speculation. The dominant view, however, is that collapsing neutron stars become black holes – objects with such gravity that even light cannot escape them.

The lightest black holes known are about five times more massive than the Sun. Significantly more than the 2.2 times required for a neutron star to collapse. The difference in mass between the most massive neutron stars and the lightest black holes is called 'the black hole mass gap'.

Read more about the new discovery

The finding was published in the prestigious journal Science: https://www.science.org/doi/10.1126/science.adg3005

Also see the press release from the Max Planck Institute: https://www.mpg.de/21385526/0115-radi-lightest-black-hole-or-heaviest-neutron-star-150300-x