搜索结果: 1-15 共查到“原子核物理学 Neutron”相关记录78条 . 查询时间(0.511 秒)
China and Russia sign fast-neutron reactors cooperation agreement（图）
中俄 快中子堆 合作协议
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2023/3/29
Russia's Rosatom and China's Atomic Energy Authority (CAEA) have signed a Comprehensive Programme for Long-Term Cooperation in the field of fast-neutron reactors and closing the nuclear fuel cycle.
2017中子散射戈登研讨会（The 2017 Gordon Research Conference on Neutron Scattering）
2017 中子散射戈登 研讨会
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2017/1/11
With major new investments in infrastructure for neutron science in the US, Europe, Asia, and Australia either completed or in advanced planning, our capabilities for understanding new materials using...
Protons hog the momentum in neutron-rich nuclei（图）
neutron-rich nuclei Protons hog
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2014/12/1
NEWPORT NEWS, VA, October 16, 2014 – Like dancers swirling on the dance floor with bystanders looking on, protons and neutrons that have briefly paired up in the nucleus have higher-average momentum, ...
Protons hog the momentum in neutron-rich nuclei
neutron-rich nuclei Protons hog
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2014/10/30
NEWPORT NEWS, VA, October 16, 2014 – Like dancers swirling on the dance floor with bystanders looking on, protons and neutrons that have briefly paired up in the nucleus have higher-average momentum, ...
Upper limits on the observational effects of nuclear pasta in neutron stars
relativity – gravitational waves – dense matter – stars neutron – stars
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2011/7/21
The effects of the existence of exotic nuclear shapes at the bottom of the neutron star inner crust - nuclear `pasta' - on observational phenomena are estimated by comparing the limiting cases that th...
QHD equation of state for strongly magnetized neutron stars
QHD equation strongly magnetized neutron stars
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2011/7/21
We investigate the quantum hadrodynamic equation of state for neutron stars (with and without including hyperons) in the presence of strong magnetic fields.
Oscillations of hot, young neutron stars: Gravitational wave frequencies and damping times
Oscillations of hot young neutron stars
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2011/7/21
We study how the frequencies and damping times of oscillations of a newly born, hot proto-neutron star depend on the physical quantities which characterize the star quasi-stationary evolution which fo...
A model for space and time-like proton (neutron) form factors
space time-like proton (neutron)
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2011/7/21
Recent experiments on the electromagnetic proton and neutron form factors reveal very peculiar features such as the decreasing of the ratio of electric to magnetic form factor of the proton as functio...
A model for space and time-like proton (neutron) form factors
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2011/7/21
Recent experiments on the electromagnetic proton and neutron form factors reveal very peculiar features such as the decreasing of the ratio of electric to magnetic form factor of the proton as functio...
Multi-messenger observations of neutron rich matter
Multi-messenger neutron rich matter
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2011/7/21
Neutron rich matter is central to many fundamental questions in nuclear physics and astrophysics. Moreover, this material is being studied with an extraordinary variety of new tools such as the Facili...
Study of the neutron skin thickness of ${}^{208}$Pb in mean field models
mean field models
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2011/7/20
We study whether the neutron skin thickness $\Delta r_{np}$ of ${}^{208}$Pb originates from the bulk or from the surface of the neutron and proton density distributions in mean field models.
Relativistic separable interaction kernel of the neutron-proton system with inelasticities
neutron-proton system Relativistic separable interaction
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2011/7/20
Within a covariant Bethe-Salpeter approach, the relativistic complex separable neutron-proton interaction kernel is proposed. The uncoupled partial-wave states with the total angular momentum $J$=0,1 ...
Emergence of pygmy dipole resonances: Magic numbers and neutron skins
pygmy dipole resonances Magic numbers neutron skins
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2011/7/20
The pygmy dipole resonances (PDR) for even-even nuclei in 8=erforming a systematic calculation of the random-phase approximation with the Skyrme functional of SkM*. The calculation...
Testing the density matrix expansion against ab initio calculations of trapped neutron drops
density matrix neutron drops
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2011/7/20
Microscopic input to a universal nuclear energy density functional can be provided through the density matrix expansion (DME), which has recently been revived and improved.
Constraining the neutron-neutron scattering length with \eftnopi
neutron-neutron scattering length
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2011/7/20
We compute a model-independent correlation between the difference of neutron-neutron and proton-proton scattering lengths |a(nn)-a^C(pp)| and the splitting in binding energies between Helium-3 and tri...