Neutron stars form when a large star's core collapses, and the atoms collapse under the weight of gravity to form a dense sea of neutrons.
The equation of state of neutron matter indicates that the upper mass limit for a neutron star should be around 2.2 to 2.6 solar masses.
Since neutron stars are rotating, we can measure their rate of rotation.
Some physicists and astronomers have suggested that quarks might break free in a neutron star's dense heart to create a quark star.
Pulsars, which emit radio pulses, rotate at frequencies that can reveal the minimum density for the object to remain intact.
Millisecond pulsars can rotate above 700 Hz, and their density in polar regions is higher than near the equator, raising questions of whether the polar areas might contain quark matter.
A better fit for the fastest pulsars was obtained by comparing a traditional equation of state model to a hybrid model, which included both neutron and quark matter.
Currently observed millisecond pulsars can be described by the traditional model, but higher rotation frequency indicating quark matter would shift the upper limit to 1,000 rotations a second.
More millisecond pulsars with a wide range of masses would reveal how rotation frequency varies with mass at the upper limit and which of the two models the data strengthens.
These findings were published in a research paper titled “Fastest spinning millisecond pulsars: indicators for quark matter in neutron stars?” on arXiv(pre-print server).