A new model for matter in neutron star collisions. After a massive star burns its fuel and explodes as a supernova, an exceedingly compact object known as a neutron star may form. Neutron stars are very dense: to get the density within them, one would have to shrink a large body like our sun to the
A new model for matter in neutron star collisions.
The Asia Pacific Center for Theoretical Physics in Pohang, South Korea, Dr. Matti Järvinen, Dr. Tuna Demircik, and Dr. Christian Ecker from the Institute for Theoretical Physics ofFrankfurt, Germany, have now created a new model that allows them to GET one step closer to answering this question. They combine models from nuclear physics, which are not applicable at high densities, with a method employed in string theory to describe the transition to dense and hot quark matter.
“Our method uses a mathematical relationship found in string theory, namely the correspondence between five-dimensional black holes and strongly interacting matter, to describe the phase transition between dense nuclear and quark matter,” explains Dr. Demircik and Dr. Järvinen.
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