NEUTRON STARS – SCI & TECH

News: Evidence grows for deconfined quark matter in neutron-star cores

 

What's in the news?

       Neutron stars are the collapsed cores of stars that pack more than a Sun’s worth of matter into objects just 10–20 km in radius.

       The density of a neutron star is expected to increase from its crust to its core. As a result electrons and protons in the interior of such a star are expected to be crushed together to create matter that is mostly neutrons.

 

Neutron Stars:

       Neutron stars are some of the most fascinating and mysterious celestial objects in the universe.

       Formed from the remnants of massive stars during supernova explosions, these incredibly dense and compact entities have captivated the minds of astronomers and physicists alike.

 

Backdrop:

       Neutron stars are the incredibly dense remnants left behind after a massive star undergoes a supernova explosion.

       These stellar corpses are composed almost entirely of neutrons packed together with unimaginable density.

 

Formation of Neutron Stars:

       The formation of a neutron star begins with a massive star, typically several times more massive than our Sun, nearing the end of its life. When such a star exhausts its nuclear fuel, it can no longer support itself against gravitational collapse.

       The star then undergoes a catastrophic explosion known as a supernova, releasing an enormous amount of energy.

       During this explosion, the outer layers of the star are expelled into space, while the core collapses in on itself, forming a neutron star.

 

Characteristics of Neutron Stars:

1. Mass and Size:

       Neutron stars are incredibly compact, with masses ranging from about 1.4 to 3 times that of our Sun. However, their small size is truly remarkable.

       Despite their immense mass, neutron stars have diameters of only around 10-20KM.

2. Density:

       Neutron stars are the densest objects known in the universe. The density of their core is mind-boggling, surpassing even the densities found in atomic nuclei.

       A neutron star’s matter is so tightly packed that protons and electrons combine to form neutrons, hence the name.

3. Gravitational Pull:

       Due to their high mass and compact size, neutron stars have an incredibly strong gravitational pull.

       It is estimated that if an object were to fall from a height of just one meter above the surface of a neutron star, it would hit the surface with roughly one-third of the speed of light.