
The collision and merger of two neutron stars—the extremely dense remnants of collapsed stars—are among the most energetic occasions within the universe, producing quite a lot of indicators that may be noticed on Earth.
New simulations of neutron star mergers by a staff from Penn State and the College of Tennessee Knoxville reveal that the blending and altering of tiny particles known as neutrinos that may journey astronomical distances undisturbed impacts how the merger unfolds, in addition to the ensuing emissions. The findings have implications for longstanding questions in regards to the origins of metals and uncommon earth components in addition to understanding physics in excessive environments, the researchers stated.
The paper, printed within the journal Physical Review Letters, is the primary to simulate the transformation of neutrino “flavors” in neutron star mergers. Neutrinos are basic particles that work together weakly with different matter, and are available in three flavors, named for the opposite particles they affiliate with: electron, muon and tau. Underneath particular situations, together with the within of a neutron star, neutrinos can theoretically change flavors, which might change the sorts of particles with which they work together.
“Earlier simulations of binary neutron star mergers haven’t included the transformation of neutrino taste,” stated Yi Qiu, graduate scholar in physics within the Penn State Eberly Faculty of Science and first writer of the paper.
“That is partly as a result of this course of occurs on a nanosecond timescale and may be very troublesome to seize and partly as a result of, till not too long ago, we did not know sufficient in regards to the theoretical physics underlying these transformations, which falls outdoors of the usual mannequin of physics.
“In our new simulations, we discovered that the extent and placement of neutrinos mixing and reworking impacts the matter that’s ejected from the merger, the construction and composition of what stays after the merger—the remnant—in addition to the fabric round it.”
The researchers constructed a pc simulation of a neutron star merger from the bottom up, incorporating quite a lot of bodily processes, together with gravity, normal relativity, hydrodynamics and the neutrino mixing. Additionally they accounted for the transformation of electron taste neutrinos to muon taste, which the researchers stated is essentially the most related neutrino transformation on this surroundings. They modeled a number of situations, various the timing and placement of the blending in addition to the density of the encompassing materials.
The researchers discovered that each one of those elements influenced the composition and construction of the merger remnant, together with the kind and portions of components created through the merger. Throughout a collision, the neutrons in a neutron star may be launched at different atoms within the particles, which might seize the neutrons and finally decay into heavier components, comparable to heavy metals like gold and platinum in addition to uncommon earth components which might be used on Earth in sensible telephones, electrical car batteries and different units.
“A neutrino’s taste adjustments the way it interacts with different matter,” stated David Radice, Knerr Early Profession Professor of Physics and affiliate professor of astronomy and astrophysics on the Penn State Eberly Faculty of Science and an writer of the paper. “Electron sort neutrinos can take a neutron, one of many three fundamental components of an atom, and rework it into the opposite two, a proton and electron. However muon sort neutrinos can not do that.
“So, the conversion of neutrino flavors can alter what number of neutrons can be found within the system, which instantly impacts the creation of heavy metals and uncommon earth components. There are nonetheless many lingering questions in regards to the cosmic origin of those vital components, and we discovered that accounting for neutrino mixing might enhance component manufacturing by as a lot as an element of 10.”
Neutrino mixing through the merger additionally influenced the quantity and composition of matter ejected from the merger, which the researchers stated might alter the emissions detectable from Earth. These emissions usually embrace gravitational waves—ripples in area time—in addition to electromagnetic radiation like X-rays or gamma rays.
“In our simulations, neutrino mixing impacted the electromagnetic emissions from neutron star mergers and presumably the gravitational waves as nicely,” Radice stated.
“With cutting-edge detectors like LIGO, Virgo and KAGRA and their next-generation counterparts, such because the proposed Cosmic Explorer observatory that might begin operations within the 2030s, astronomers are poised to detect gravitational waves extra usually than we now have earlier than. Higher understanding how these emissions are created from neutron star mergers will assist us interpret future observations.”
The researchers stated modeling the blending processes was much like a pendulum being turned the wrong way up. Initially, many adjustments occurred on an extremely speedy timescale, however ultimately the pendulum settles to a secure equilibrium. However a lot of this, they stated, is an assumption.
“There’s nonetheless quite a bit we do not know in regards to the theoretical physics of those neutrino transformations,” Qiu stated. “As theoretical particle physics continues to advance, we will drastically enhance our simulations. What stays unsure is the place and the way these transformations happen in neutron star mergers. Our present understanding suggests they’re very doubtless, and our simulations present that, in the event that they happen, they will have main results, making it vital to incorporate them in future fashions and analyses.”
Now that the infrastructure for these advanced simulations has been created, the researchers stated they count on different teams will use the expertise to proceed to discover the impacts of neutrino mixing.
“Neutron star mergers operate like cosmic laboratories, offering vital insights into excessive physics that we won’t replicate safely on Earth,” Radice stated.
Along with Qiu and Radice, the analysis staff contains Maitraya Bhattacharyya, postdoctoral scholar within the Penn State Institute for Gravitation and the Cosmos, and Sherwood Richers on the College of Tennessee, Knoxville.
Extra data:
Yi Qiu et al, Neutrino Taste Transformation in Neutron Star Mergers, Bodily Evaluate Letters (2025). DOI: 10.1103/h2q7-kn3v. On arXiv: DOI: 10.48550/arxiv.2503.11758
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Mixing neutrinos of colliding neutron stars adjustments how merger unfolds, simulations reveal (2025, September 21)
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