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Neutron Stars

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May 1, 2024 3 minute read

Neutron stars are the collapsed remnants of massive stars that have undergone a supernova explosion. They are incredibly dense objects, with masses that can be up to twice the mass of our Sun, but with diameters of only about 20 kilometers. This means that the material in a neutron star is squeezed together to such an extent that its atoms are crushed and the electrons are forced to combine with the protons to form neutrons. This gives neutron stars their characteristic high density.

Neutron Star Formation

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Reading list

We've selected four books that we think will supplement your learning. Use these to develop background knowledge, enrich your coursework, and gain a deeper understanding of the topics covered in Neutron Stars.
Provides a comprehensive overview of the physics of neutron stars, covering everything from their basic properties to their most extreme states. It is written by two leading experts in the field and is suitable for both researchers and advanced students.
Provides a comprehensive overview of the high-energy astrophysics of neutron stars and black holes, covering everything from the basic physics to the latest observations. It is written by six leading experts in the field and is suitable for both researchers and advanced students.
Provides a comprehensive overview of neutron stars and related phenomena, covering everything from their basic properties to their most extreme states. It is written by a leading expert in the field and is suitable for both researchers and advanced students.
Provides a detailed overview of the relationship between neutron stars and gamma-ray bursts, covering everything from the theoretical models to the observational evidence. It is written by a leading expert in the field and is suitable for both researchers and advanced students.
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