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Internal structure of Neutron Stars

Internal structure of Neutron Stars. Artistic view . Astronomy meets QCD. arXiv: 0808.1279. For NSs we can take T=0 and neglect the third equation. Hydrostatic equilibrium for a star. For a NS effects of GR are also important. M/R ~ 0.15 (M/M ? ) (R/10 km ) -1

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511 views • 36 slides

Recent Results from Super-Kamiokande on Atmospheric Neutrino Measurements

Recent Results from Super-Kamiokande on Atmospheric Neutrino Measurements. Choji Saji ICRR,Univ. of Tokyo for the Super-Kamiokande collaboration. ICHEP 2004, Beijing. Contents. Atmospheric neutrino oscillation studies using full Super-Kamiokande I(SK-I) data

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298 views • 15 slides

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Dl e - PowerPoint PPT Presentation

Internal structure of Neutron Stars

Recent Results from Super-Kamiokande on Atmospheric Neutrino Measurements