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Neutron Degeneracy

Neutron Degeneracy

Neutron degeneracy is a stellar application of the Pauli Exclusion Principle, as is electron degeneracy. No two neutrons can occupy identical states, even under the pressure of a collapsing star of ...

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http://hyperphysics.phy-astr.gsu.edu/hbase/astro/pulsar.html#c3
Neutron Stars - Introduction

Neutron Stars - Introduction

Brief introduction from NASA on the nature of neutron stars, includes links to related topics.

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http://imagine.gsfc.nasa.gov/docs/science/know_l1/neutron_stars.html
ISIS Pulsed Neutron & Muon Source

ISIS Pulsed Neutron & Muon Source

The homepage of the world's leading pulsed neutron source

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http://www.isis.rl.ac.uk/
Bertram N. Brockhouse

Bertram N. Brockhouse

Bertram N. Brockhouse (1918 - ) received the Nobel Prize for Physics in 1994 for pioneering contributions to the development of neutron scattering techniques for studies of condensed matter. In ...

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http://www.nobel.se/physics/laureates/1994/brockhouse-autobio.html
Clifford G. Shull

Clifford G. Shull

Clifford G. Shull (1915 - 2001) received the Nobel Prize for Physics in 1994 for pioneering contributions to the development of neutron scattering techniques for studies of condensed matter. In ...

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http://www.nobel.se/physics/laureates/1994/shull-autobio.html
Event Horizon

Event Horizon

After collapse to the neutron star stage, stars with masses less than 1-3 solar masses should remain neutron stars. Those of masses greater than 1 to 3 collapse toward zero spatial extent - toward a ...

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http://hyperphysics.phy-astr.gsu.edu/hbase/astro/blkhol.html#c1
Hyperphysics - Neutrons

Hyperphysics - Neutrons

Structure and stability of the neutron with good links to other relevant parts of the site.

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http://hyperphysics.phy-astr.gsu.edu/hbase/particles/proton.html#c3
Nuclear Isotope Half-Lifes

Nuclear Isotope Half-Lifes

The site demonstrates the half-life of ten basic nuclei and you can add or subtract a proton or a neutron to the current isotope.

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http://lectureonline.cl.msu.edu/~mmp//kap30/Nuclear/nuc.htm
Cygnus X-1

Cygnus X-1

Doppler studies of this blue supergiant in Cygnus indicate a period of 5.6 days in orbit around an unseen companion. The mass of the companion is calculated to be 8-10 solar masses, much too large to ...

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http://hyperphysics.phy-astr.gsu.edu/hbase/astro/blkbin.html#c1
Neutron Star

Neutron Star

For a sufficiently massive star, an iron core is formed and still the gravitational collapse has enough energy to heat it up to a high enough temperature to either fuse or fission iron. Either in the ...

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http://hyperphysics.phy-astr.gsu.edu/hbase/astro/pulsar.html#c1
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