LIGO Uncovers the Most Massive Black Hole Collision Ever Recorded

Illustration of black hole merger

Shutterstock / Jurik Peter

New records for black holes have transformed our understanding of the universe’s most extreme entities.

The Laser Interferometer Gravitational-Wave Observatory (LIGO) began its groundbreaking detection of gravitational waves—ripples in the fabric of spacetime—ten years ago, unveiling nearly 100 black hole collisions. On November 23, 2023, Rigo announced receiving a signal described as “an extraordinary interpretation that defies explanation.” According to Sophie Binnie from the California Institute of Technology, her team ultimately concluded that it corresponded to the largest black hole merger ever recorded.

One of the merging black holes was approximately 100 times the mass of the sun, while the other neared 140 solar masses. Previous records featured black holes that were almost half as massive, primarily due to earlier mergers. Team member Mark Hannam from Cardiff University, UK, emphasized that these black holes were not only immense but also spinning at such high speeds that they challenged mathematical models of the universe regarding their formation.

According to Hannam, the masses of these black holes exceed those typically formed from the collapse of aging stars, suggesting they likely resulted from earlier mergers between smaller black holes. “It’s possible that multiple mergers have occurred,” he notes.

“A decade ago, we were astonished to find black holes around 30 solar masses. Now, we observe black holes over 100 solar masses,” adds Davide Gerosa from the University of Bicocca in Milan, Italy. He mentions that gravitational wave signals from these large, quickly rotating black holes are shorter and consequently more challenging to detect. Binnie presented her findings at the Edoardo Amaldi Conference on Gravitational Waves in Glasgow, England, on July 14.

Both Hannam and Binnie emphasize that future observations of similarly remarkable mergers are essential to further decipher these new signals, including unraveling the origins of black holes. As upgrades progress, LIGO is expected to detect more cosmic record-breakers. Yet, in May, the Trump administration proposed halving resources at the facility, which, in Hannam’s opinion, could render capturing new signals exceedingly difficult.

Topic:

Source: www.newscientist.com

LIGO hunts for gravitational waves produced by mountains on neutron stars

While the solar system’s moons such as Europa and Enceladus have thin crusts over deep oceans, Mercury has a thin crust over a large metallic core. Thin sheets are generally likely to wrinkle. Europa has linear features, Enceladus has “tiger stripes” and Mercury has foliated cliffs. Neutron stars may have similar characteristics. These neutron star mountains can generate detectable oscillations in space and time known as gravitational waves, according to a new study.

Artist’s impression of a neutron star. Image credit: Sci.News.

Neutron stars are a trillion times denser than lead, and their surface features are largely unknown.

Nuclear theorists investigated the mountain-building mechanisms active on the moons and planets of the solar system.

Some of these mechanisms suggest that neutron stars likely have mountains.

A mountain in a neutron star would be much more massive than any mountain on Earth. They are so huge that the gravitational pull from these mountains alone can generate gravitational waves.

of Laser interferometer Gravitational wave observatory (LIGO) is currently looking for these signals.

“These waves are so weak that they require highly detailed and sensitive techniques carefully tuned to the expected frequencies and other signal characteristics,” said nuclear astrophysicist Jorge Morales and professor Charles Horowitz at Indiana University. It can only be discovered through search.”

“The first detection of continuous gravitational waves opens a new window on the universe and will provide unique information about neutron stars, the densest objects after black holes.”

“These signals may also provide sensitive tests of fundamental laws of nature.”

The authors investigated the similarities between neutron star mountains and surface features of solar system objects.

“While both neutron stars and certain moons, such as Jupiter’s moon Europa and Saturn’s moon Enceladus, have a thin crust over a deep ocean, Mercury has a thin crust over a large metallic core. The thin sheet Wrinkles are universally possible,” they said.

“Europa has linear features, Enceladus has tiger-like stripes, and Mercury has curved, step-like structures.”

“Mountained neutron stars may have similar types of surface features that can be discovered by observing continuous gravitational wave signals.”

“Earth’s innermost core is anisotropic, and its shear modulus is direction-dependent.”

“If the material in the neutron star’s crust is also anisotropic, a mountain-like deformation will occur, and its height will increase as the star rotates faster.”

“Such surface features could explain the maximum spin observed in neutron stars and the minimum possible deformation of radio-emitting neutron stars known as millisecond pulsars.”

team’s paper Published in a magazine Physical Review D.

_____

JA Morales and CJ Horowitz. 2024. The anisotropic neutron star crust, the mountains of the solar system, and gravitational waves. Physics. Rev.D 110, 044016; doi: 10.1103/PhysRevD.110.044016

Source: www.sci.news