Neutron star mergers tagged posts

Finding New Physics in Debris from Colliding Neutron Stars

Artist’s illustration of two merging neutron stars. (Image: National Science Foundation/LIGO/Sonoma State University/A. Simonnet)

Neutron star mergers are a treasure trove for new physics signals, with implications for determining the true nature of dark matter, according to research from Washington University in St. Louis.

On Aug. 17, 2017, the Laser Interferometer Gravitational-wave Observatory (LIGO), in the United States, and Virgo, a detector in Italy, detected gravitational waves from the collision of two neutron stars. For the first time, this astronomical event was not only heard in gravitational waves but also seen in light by dozens of telescopes on the ground and in space.

Physicist Bhupal Dev in Arts & Sciences used observations from this neutron star merger — an ev...

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NASA Missions Probe Game-Changing Cosmic Explosion

Two neutron stars begin to merge in this illustration, blasting a jet of high-speed particles and producing a cloud of debris. Scientists think these kinds of events are factories for a significant portion of the universe’s heavy elements, including gold.
Credits: A. Simonnet (Sonoma State Univ.) and NASA’s Goddard Space Flight Center

On Dec. 11, 2021, NASA’s Neil Gehrels Swift Observatory and Fermi Gamma-ray Space Telescope detected a blast of high-energy light from the outskirts of a galaxy around 1 billion light-years away. The event has rattled scientists’ understanding of gamma-ray bursts (GRBs), the most powerful events in the universe.

For the last few decades, astronomers have generally divided GRBs into two categories...

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Cosmic Heavy Metals help Scientists Trace the History of Galaxies

What is the origin of gold, silver, platinum? Credit: © alexphoto71 / Fotolia

What is the origin of gold, silver, platinum? Credit: © alexphoto71 / Fotolia

The origin of many of the most precious elements on the periodic table, such as gold, silver and platinum, has perplexed scientists for >6 decades. Now a recent study has an answer, evocatively conveyed in the faint starlight from a distant dwarf galaxy. In a roundtable discussion The Kavli Foundation spoke to 2 of the researchers behind the discovery about why the source of these heavy elements, collectively called “r-process” elements, has been so hard to crack.

“Understanding how heavy, r-process elements are formed is one of hardest problems in nuclear physics,” said Assistant/Prof Anna Frebel, MIT...

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