When a neutron star is consumed by another star, a burst of neutrinos can be generated. This burst of neutrinos might be detectable on Earth. 

Neutrinos are ghostly particles that hardly ever interact with normal matter. They are electrically neutral and have a very small rest mass. Neutrinos typically pass through normal matter unimpeded and undetected. 

Neutrinos are the driving factor for core-collapse supernovae, the violent death of massive stars. Neutrinos are responsible for transferring energy from the hot proto-neutron star (PNS) to the surrounding material. 

Neutrino detectors are often built underground to isolate the detector from cosmic rays and other background radiation.

It seems consuming partners is not unheard of. It’s even seen in the lives of stars where binary stars orbit one another closely and one star ultimately consumes the other. If the victim is a neutron star a burst of neutrinos can be generated and a new study reveals they might just be detectable on Earth.

A neutron star is formed when a massive star runs out of fuel and collapses. The core of the star collapses, crushing every proton and electron into a neutron. The hydrogen nuclei (protons) absorb electrons and become neutrons, releasing neutrinos in the process. 

Neutron stars emit neutrinos to cool down. Instead of emitting light, they emit neutrinos. Neutron stars may fire out neutrinos in beams like a laser light show. 

Neutrinos are also copiously emitted by neutron star mergers, due to the high temperatures reached by dense matter during the merger and its aftermath

Yes, most neutrinos will pass completely through a neutron star as though it were not even there. Neutrinos interact very weakly with matter and pass through most of it undisturbed. 

Neutron stars are transparent to their own thermally produced neutrinos and any other neutrinos of energies below a few MeV once they have cooled to highly degenerate states at temperatures of ≤1010 K. 

Neutrinos are a very efficient cooling mechanism for a neutron star, carrying energy away from the outermost layer of the crust.

Neutron stars can cool down over millions of years. They radiate heat, which is called radiational cooling. Over time, most lone neutron stars fade away and become essentially invisible. 

Neutron stars can also merge with other neutron stars or black holes. This can create a black hole or a more massive neutron star. 

Neutron stars can also be destroyed by black holes. Black holes can accrete material at the center of a neutron star and eventually swallow the entire star. 

Neutron stars can also explode in a supernova. This happens when a neutron star can no longer produce enough energy to maintain its structure and collapses under its own gravitational pressure. 

Neutron stars can also become hydrogen stars. This happens when a neutron star is heated sufficiently, it becomes non-degenerate. Eventually, the neutrons decay and it becomes a hydrogen star.

Yes, neutron stars produce antimatter: 

• Matter-antimatter pairs Neutron stars produce large amounts of matter-antimatter pairs. 
• Pulsars Pulsars, which are young, rapidly rotating neutron stars, produce a powerful matter/anti-matter wind. 
• Laser pincers Physicists have created antimatter by firing two lasers at each other to recreate the conditions near a neutron star. 
• Jets Black holes and neutron stars produce vast amounts of positron-electron plasma via the jets. 

Neutron stars are one of the most steady sources of antimatter that we know of. The incredible gravity of a dying star greatly condenses the protons and neutrons in its core. 

Antimatter does not exist on Earth except for the small fraction of antimatter which can be found in controlled lab environments and is produced by humans

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