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In nuclear physics, "magic numbers" identify specific numbers of protons or neutrons that lead to especially stable nuclei.
Researchers currently think that the dividing line between neutron stars and black holes lies much closer to 3 times the mass of the sun than 5 times the mass of the sun (Green, Jones, 2015, pg 251).
The neutron star, known as PSR J0952-0607, was discovered in 2017 about 3,000 light-years from Earth in the constellation Sextans. Recent measurements show the star weighs 2.35 times as much as ...
Small but Mighty. Despite their small diameters—about 12.5 miles (20 kilometers)—neutron stars boast nearly 1.5 times the mass of our sun, and are thus incredibly dense.
Double-column spectrometer remedies traditional shortcomings to drastically improve counting efficiency and resolution ...
"The study makes it plausible that the mysterious low-mass object of 1.17 solar masses in system J0453+1559 is indeed a neutron star and not a white dwarf, as some authors have recently proposed ...
Recent theoretical and experimental advances provide new insights into how mass is distributed within particles like protons, neutrons, and pions, offering critical guidance for future research ...
The researchers said the neutron star, wildly spinning at 707 times per second, has a mass about 2.35 times greater than that of our sun, putting it perhaps at the maximum possible mass for such ...
Fifty experts on nuclear physics, particle physics and astrophysics met at CERN from 9 to 13 June to discuss how to use ...
The neutron star featured in this latest paper is a pulsar, PSR J0952-0607—or J0952 for short—located in the constellation Sextans between 3,200 and 5,700 light-years away from Earth.
Scientists determined that one of the two merging objects had a mass between 1.2 to 2 times the mass of our sun—most likely a neutron star—while the other's mass fell in the mass-gap range of ...
A computer simulation shows how two neutron stars of unequal mass merge, form a black hole and spit out a jet of high energy matter.