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The concept of this artist depicts magnetic – a type of neutron stars with a strong magnetic field. | Credit: NASA/JPL-Caltech
Neutrino stars are some of the strangest cosmic things, and the greatest puzzles lie in the depths of their hearts.
Neutron stars It is the remaining cores of explosive stars and the most known material in the universe. The typical neutron star has a mass several times Sun blockCompressed in the area only tens of one kilometers across. In the outer layers of neutron stars, the density is greater than the density of diamonds. In the nuclei of the neutron stars, cracker pressures can be pressed on atomic nuclei, and perhaps even Protons and Neutrons themselves.
The surface weight of the neutron stars is so intense that the largest “mountains” are only a few millimeters long. And those surfaces are already strange, consisting of a shell of heavy atomic nuclei that was pressed in a crystal network with Electrons Free swimming between them.
Deeper to the bottom, the huge attractiveness It is allowed to have strange and rare isotopes in abundance. Usually, you can only cram a lot of neutrons in a nucleus before it only collapses, due to the hateful effects of Strong nuclearity Funding firmness. But the danger of the neutron star keeps everything binding together. To approximately a kilometer, the atomic nucleus can carry hundreds of neutrons at one time.
But even this has an end. A little more than half a mile (1 km) in the depth, even those nuclei of impossible size. This is the “dotting line”, where neutrons begin to leak from the core. Usually, any free neutrons decompose in about 15 minutes. But the intense boundaries of the neutron star keep the neutrons stable and free flow.
After about one mile (2 km) in the depth of the neutron star, the substance may take its strangest forms so far: “nuclear pasta”. In this region, where the dandruff is transmitted to the basic forces, the vital forces – gravity, strong nuclear power and electrical crowding – compete for dominance. This leads to an exaggerated strange nuclei in exaggerated shapes, known as Gnocchi.
Below, the individual blocs are pressed together in long tubes (relatively from the relatively; everything here is still microscopy), known as spaghetti. After that, the spaghetti is combined together to form the lasagna, which then merges into one uniform mass. But this bloc has defects and holes in it – “AntiSpaghetti” and “Antignocchi”.
Finally, the thickness of the nuclear pasta area is only about 330 feet (100 meters), but it weighs more than 3000 lands. This is a lot of pasta.
The neutron star can be the size of New York City with a larger mass. Quark will be more intense theoretical. | Credit: NASA/Godard Space Flight
Below, at a depth of about a mile, the nuclei simply collapses, as it is unable to maintain its structures in the overwhelming environment. Here, neutrons, protons and some electrons roam freely. What really happens in the main area of the neutron star is the issue of a lot of discussion, because physics here exceeds our current understanding.
We strongly doubt that the outer area of the nucleus is super extreme, as the neutrons are free to move with zero viscosity and zero friction. The remaining protons in this depth are now a super connector, with no electrical resistance. In these depths, the density is similar to the atomic nucleus, where the protons and neutrons are tightly pressed as possible. This area of the neutron star, for all intentions and purposes, is a single microscopic atomic nucleus, does not result in strong nuclear power but by absolute gravity.
In this region, the neutron makes a large part of the star supporting more gravitational collapse. One of the methods is the “decline pressure”-it is tightly compressed together that it explodes at incredible speeds close to lighting, creating pressure. Besides, strong nuclear force is disgusting between neutrons, which prevents them from pressing more together.
In the deepest areas of the heart, however, we have no simply idea. The density in the heart of the depth is higher than the atomic nucleus. We have no hope to repeat or re -create these conditions in the laboratory, so we only have blurry sports models to guide us. In some models, neutrons maintain their superior state.
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In other models, various forms of the material – such as hyperons, deledas and boson condensate – may arise. This is possible because neutrons and protons are made of smaller molecules, called Quarks. In these circumstances, quarks may be arranged and combined differently in situations that will be immediately unstable in any other environment. But here, you may be completely fine.
In other models, all protons and neutrons – and even their most strange cousins - completely collapse, form a soup of quarks GaglonStrong nuclear power holders.
But all this is pure speculation. The nearest Neitron star is located hundreds of light years away, and even if we can open it, the special circumstances that create these types of strange conditions will collapse. Therefore, at the present time, the only way to form neutron stars is mathematics and a heavy dose of guessing.
