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Astrophysics Breakthrough: The Fate of Neutron Star Merger Remnants

Astrophysics Breakthrough: The Fate of Neutron Star Merger Remnants

August 7, 2024
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Astrophysics Breakthrough: The Fate of Neutron Star Merger Remnants

by nasaspacenews
August 7, 2024
in News, Others, Solar System
0
Astrophysics Breakthrough: The Fate of Neutron Star Merger Remnants

An illustration of two neutron stars merging, along with the resulting gravitational waves [NASA's Goddard Space Flight Center]

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Neutron star mergers have long captivated scientists, and recent breakthroughs have illuminated the aftermath of these colossal cosmic collisions. When two neutron stars collide, they create a remnant teeming with secrets about the universe. The latest research from Pennsylvania State University is particularly groundbreaking. By utilizing supercomputer simulations with general-relativistic neutrino-radiation hydrodynamics, these scientists have delved into the enigmatic remnants of neutron star mergers. This advanced modeling reveals the intricate cooling process of the remnant, which emits neutrinos—a type of elementary particle. Unlike typical stars, the remnant’s surface temperature surpasses that of its core, creating a unique scenario where convective plumes are unlikely to form.The central object of the remnant, which contains most of the mass, is surrounded by a fast-rotating ring of hot matter. This configuration plays a significant role in the remnant’s evolution and stability.

Scientists have used supercomputer simulations to study gravitational waves produced by merging neutron stars, revealing a correlation between the remnant temperature and wave frequency. These findings are significant for future gravitational-wave detectors, which will differentiate between models of hot nuclear matter. Credit: SciTechDaily.com

As the remnant cools by emitting neutrinos, it generates a distinctive signature detectable by observatories on Earth. This crucial information enables astronomers to pinpoint neutron star mergers’ locations and meticulously study their properties. Moreover, these findings pave the way for future observations and theoretical models, significantly enhancing our ability to explore the universe.

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The significance of this study extends beyond the realm of astrophysics. By unraveling the mysteries of neutron star merger remnants, scientists can gain insights into the fundamental laws of physics. This research contributes to our understanding of the strong force, one of the four fundamental forces in nature, and its role in the behavior of nuclear matter. Additionally, it provides a framework for studying other extreme astrophysical phenomena, such as supernovae and black holes. 

The study published in The Astrophysical Journal utilized resources from the Department of Energy’s National Energy Research Scientific Computing Center, the Leibniz Supercomputing Center in Germany, and the Institute for Computational and Data Science at Pennsylvania State University. 

FEATURED POST

This Hubble image shows Omega Centauri, the Milky Way's largest globular clusters. Globular clusters contain some of the oldest stars in the Universe, and new research determines their absolute age. Image Credit: ESA/Hubble & NASA, M. Häberle (MPIA)

Astronomers Just Unlocked the Birth Dates of the Milky Way’s Oldest Stars

May 12, 2025
Image NASA’s Solar Dynamics Observatory captured this image of the Sun on May 7, 2024

There’s a Violent Solar Storm That Could Have Been Worse—Here’s the Scary Truth

May 11, 2025
This six-panel illustration of a tidal disruption event around a supermassive black hole shows the following: 1) A supermassive black hole is adrift inside a galaxy, its presence only detectable by gravitational lensing; 2) A wayward star gets swept up in the black hole's intense gravitational pull; 3) The star is stretched or "spaghettified" by gravitational tidal effects; 4) The star's remnants form a disk around the black hole; 5) There is a period of black hole accretion, pouring out radiation across the electromagnetic spectrum, from X-rays to radio wavelengths; and 6) The host galaxy, seen from afar, contains a bright flash of energy that is offset from the galaxy's nucleus, where an even more massive black hole dwells. Credit: NASA, ESA, STScI, Ralf Crawford (STScI)

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This Hubble image shows Omega Centauri, the Milky Way's largest globular clusters. Globular clusters contain some of the oldest stars in the Universe, and new research determines their absolute age. Image Credit: ESA/Hubble & NASA, M. Häberle (MPIA)

Astronomers Just Unlocked the Birth Dates of the Milky Way’s Oldest Stars

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