Results 261 to 270 of about 202,682 (289)

Magnetized neutron matter and deformed neutron stars

Journal of Physics G: Nuclear and Particle Physics, 2019
In this work, we study the influences of density-dependent magnetic field on the equation of state (EoS) of neutron matter using the lowest order constraint variational method. We consider the effects of neutron mass reduction due to the strong magnetic field on the EoS and perform our calculations applying magnetic field-dependent neutron mass (MFD ...
M Zamani, M Bigdeli
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Neutrons Matter

Abstract The nuclear force is key to the existence of life. The sun shines due to nuclear reactions, and there would be no life without the sun’s energy. Subtle aspects of the nuclear force are also important for life. The fact that the neutron is very slightly heavier than the proton is essential to the existence of hydrogen, the sun’s ...
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Interaction of Neutrons with Matter

2009
This chapter addresses neutron interactions with absorber atoms. Neutrons, by virtue of their neutrality, are indirectly ionizing radiation exhibiting, similarly to photons, a quasi-exponential penetration into an absorber. They deposit energy in absorber through a two-step process: energy transfer to heavy charged particles and energy deposition in ...
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Neutrons in Disordered Matter

Physica Scripta, 1995
The second in a series of Euroconferences on the use of neutrons for studies of condensed matter was arranged 9th to 13th of June 1994 at the Wijk conference center in the Stockholm archipelago. The Euroconference was sponsored by the Commission of the European Communities, Nobel Committees for Physics and Chemistry of the Royal Swedish Academy of ...
Monique Dahlborg, Ulf Dahlborg
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Magnetization of neutron matter

AIP Conference Proceedings, 2011
In this paper, we compute magnetization of neutron matter at strong magnetic field using the lowest order constrained variational (LOCV) technique.
M. Bigdeli, Ersin Göğüş, Ünal Ertan, Tomaso Belloni   +3 more
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Neutron Interaction with Matter

1992
The design and operation of a nuclear reactor requires the ability to determine how neutrons are distributed within a reactor core. This can be achieved by deriving and solving “neutron balance” equations which include all the relevant neutron loss and gain rates.
K. Almenas, R. Lee
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Constraining neutron-star matter with microscopic and macroscopic collisions

Nature, 2022
Sabrina Huth, M W Coughlin, Ingo Tews
exaly  

Neutron matter

Nuclear Physics A, 1970
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Neutron Stars and the Nuclear Matter Equation of State

Annual Review of Nuclear and Particle Science, 2021
James M Lattimer
exaly  

Neutron matter

Soviet Atomic Energy, 1972
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