'Direct urca' presentation slideshows

Direct urca - PowerPoint PPT Presentation

Neutron Stars 3: Thermal evolution

Neutron Stars 3: Thermal evolution

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568 views • 45 slides
Lead ( P b) R adius Ex periment : PREX

Lead ( P b) R adius Ex periment : PREX

Lead ( P b) R adius Ex periment : PREX. 208. E = 850 MeV , electrons on lead. Elastic Scattering Parity Violating Asymmetry. 0. Z of Weak Interaction :. Clean Probe Couples Mainly to Neutrons. ( T.W. Donnelly, J. Dubach, I Sick ).

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594 views • 44 slides
Lead ( P b) R adius Ex periment : PREX

Lead ( P b) R adius Ex periment : PREX

Lead ( P b) R adius Ex periment : PREX. 208. E = 850 MeV , electrons on lead. Elastic Scattering Parity Violating Asymmetry. 0. Z of Weak Interaction :. Clean Probe Couples Mainly to Neutrons. ( T.W. Donnelly, J. Dubach, I Sick ).

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413 views • 40 slides
Isovector Equation-of-State

Isovector Equation-of-State

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594 views • 33 slides
COOLING N EUTRON ST A R S: THEORY AND OBSERVATIONS

COOLING N EUTRON ST A R S: THEORY AND OBSERVATIONS

COOLING N EUTRON ST A R S: THEORY AND OBSERVATIONS. D.G. Yakovlev. Ioffe Physical Technical Institute, St.-Petersburg, Russia. Introduction Neutrino emission Cooling theory Phenomenological concept Theory and observation Connections Conclusions. Main collaborators:

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575 views • 30 slides
COOLING N EUTRON ST A R S: THEORY AND OBSERVATIONS

COOLING N EUTRON ST A R S: THEORY AND OBSERVATIONS

COOLING N EUTRON ST A R S: THEORY AND OBSERVATIONS. D.G. Yakovlev. Ioffe Physical Technical Institute, St.-Petersburg, Russia. Introduction Neutrino emission Cooling theory Phenomenological concept Theory and observation Connections Conclusions. Main collaborators:

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425 views • 30 slides
Lead ( P b) R adius Ex periment : PREX

Lead ( P b) R adius Ex periment : PREX

Lead ( P b) R adius Ex periment : PREX. 208. E = 850 MeV , electrons on lead. Elastic Scattering Parity Violating Asymmetry. 0. Z of Weak Interaction :. Clean Probe Couples Mainly to Neutrons. ( T.W. Donnelly, J. Dubach, I Sick ).

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388 views • 26 slides
COOLING OF N EUTRON ST A R S

COOLING OF N EUTRON ST A R S

COOLING OF N EUTRON ST A R S. D.G. Yakovlev. Ioffe Physical Technical Institute, St.-Petersburg, Russia. 1. Formulation of the Cooling Problem 2. Superlfuidity and Heat Capacity 3. Neutrino Emission 4. Cooling Theory versus Observations. History Cooling stages

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451 views • 23 slides
Nuclear Isovector Equation-of-State (EOS) and Astrophysics

Nuclear Isovector Equation-of-State (EOS) and Astrophysics

Nuclear Isovector Equation-of-State (EOS) and Astrophysics. Hermann Wolter Dep. f. Physik, LMU. Topics: Phase diagram of strongly interacting matter and exploration via heavy ion collisions Symmetric and asymmetric EoS, density dependence of symmetry energy

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243 views • 17 slides

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