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Evolution with decaying and re-emerging magnetic field

Evolution with decaying and re-emerging magnetic field

Evolution with decaying and re-emerging magnetic field. Diversity of young neutron stars. Young isolated neutron stars can appear in many flavors: Radio pulsars Compact central X-ray sources in supernova remnants. Anomalous X-ray pulsars Soft gamma repeaters

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829 views • 81 slides
Isolated Neutron Stars: News and Views

Isolated Neutron Stars: News and Views

Isolated Neutron Stars: News and Views. Sergei Popov (SAI MSU). Good old classics. For years two main types of NSs have been discussed: radio pulsars and accreting NSs in close binary systems. The pulsar in the Crab nebula. A binary system. The old zoo of neutron stars.

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742 views • 60 slides
Evolution with decaying and re-emerging magnetic field

Evolution with decaying and re-emerging magnetic field

Evolution with decaying and re-emerging magnetic field. Diversity of young neutron stars. Young isolated neutron stars can appear in many flavors: Radio pulsars Compact central X-ray sources in supernova remnants. Anomalous X-ray pulsars Soft gamma repeaters

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495 views • 39 slides
Great unification for neutron stars: The last element?

Great unification for neutron stars: The last element?

Great unification for neutron stars: The last element?. Sergei Popov SAI MSU. Diversity of young neutron stars. Young isolated neutron stars can appear in many flavors: Radio pulsars Compact central X-ray sources in supernova remnants. Anomalous X-ray pulsars Soft gamma repeaters

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513 views • 37 slides
Extensive population synthesis studies of isolated neutron stars with magnetic fi eld decay

Extensive population synthesis studies of isolated neutron stars with magnetic fi eld decay

Extensive population synthesis studies of isolated neutron stars with magnetic fi eld decay. Sergei Popov (SAI MSU) J.A. Pons, J.A. Miralles, P.A. Boldin, B. Posselt. MNRAS (2009) arXiv: 0910.2190. Diversity of young neutron stars. Young isolated neutron stars can appear in many flavors:

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408 views • 29 slides
Magnet Setup Cycling for LHC

Magnet Setup Cycling for LHC

Magnet Setup Cycling for LHC. Magnet Setup Cycling for LHC R. Wolf for the FQWG et al. Contents -Overview -Details of individual cycles -Synchronization. Aim of the magnet setup Cycling. Aims of the magnet setup cycling :

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445 views • 27 slides
Young isolated neutron stars: magnetic field decay and evolutionary links

Young isolated neutron stars: magnetic field decay and evolutionary links

Young isolated neutron stars: magnetic field decay and evolutionary links. Sergei Popov (SAI MSU). Diversity of young neutron stars. Young isolated neutron stars can appear in many flavours: Compact central X-ray sources in supernova remnants. Anomalous X-ray pulsars

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376 views • 24 slides
Unifying neutron stars

Unifying neutron stars

Unifying neutron stars. Sergei Popov (SAI MSU) in collaboration with: Andrei Igoshev (SPbSU), and Roberto Turolla (Univ. Padova). Diversity of young neutron stars. Young isolated neutron stars can appear in many flavors: Radio pulsars Compact central X-ray sources

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349 views • 18 slides
Unifying neutron stars

Unifying neutron stars

Unifying neutron stars. Sergei Popov (SAI MSU) in collaboration with: Andrei Igoshev (SPbSU), and Roberto Turolla (Univ. Padova). Diversity of young neutron stars. Young isolated neutron stars can appear in many flavors: Radio pulsars Compact central X-ray sources

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188 views • 18 slides
Evolution with decaying magnetic field

Evolution with decaying magnetic field

Evolution with decaying magnetic field. Magnetic field decay. Magnetic fields of NSs are expected to decay due to decay of currents which support them. Crustal field of core field? It is easy to decay in the crust. In the core the filed is in the form of superconducting vortices.

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264 views • 17 slides
Accreting isolated neutron stars

Accreting isolated neutron stars

Accreting isolated neutron stars. Magnetic rotator. Observational appearances of NSs (if we are not speaking about cooling) are mainly determined by P, Pdot, V, B, (also, probably by the inclination angle ? ), and properties of the surrounding medium.

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267 views • 13 slides

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