1 / 12

Cosmological Seed Fields versus Seed Fields Generated in Protogalaxies

Galactic Magnetism –Perspectives of Observation and Modeling May 16 - 20 , 201 1 Pushchino, Moscow region, Russia. Cosmological Seed Fields versus Seed Fields Generated in Protogalaxies. Dmitry Sokoloff Moscow State University Moscow, Russia in collaboration with D.Moss and V.Semikoz.

Télécharger la présentation

Cosmological Seed Fields versus Seed Fields Generated in Protogalaxies

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Galactic Magnetism –Perspectives of Observation and ModelingMay 16 - 20, 2011Pushchino, Moscow region, Russia Cosmological Seed Fields versus Seed Fields Generated in Protogalaxies Dmitry Sokoloff Moscow State University Moscow, Russia in collaboration with D.Moss and V.Semikoz

  2. GALACTIC DYNAMO Ω BT Br Basic mechanism Differential rotation α Br BT Helicity • The excitation mechanism requires a seed magnetic field. • Two options: • Magnetic field is created in after recombination • A cosmological seed field • How to decide which option is better?

  3. A standard approach: formulate scenarios for both cases, isolate specific features and try to confront them with observations A scenario for magnetic fields created after recombination: talks of Moss, Arshakian, …

  4. Seeds in protogalaxies + conventional mean-field dynamo

  5. Spatial configurations

  6. Cosmological seeds (a standard viewpoint) • Homogeneous magnetic field. • Do not destroy isotropy provided is weak enough (< 1011G is more then sufficient). • Still can be strong enough to be a seed

  7. Homogeneous relic field+ dynamo: it works unexpectedly bad (simulations of D.Moss)

  8. Rotation expels homogeneous field on the remote part of the galaxy(simulations of D.Moss)

  9. A cosmological magnetic field is useful to explain the baryon asymmetrySemikoz, Sokoloff, Valle,PRD 2009

  10. We can not distinguish between • Small-scale cosmological seed + dynamo • A battery mechanism + small scale dynamo + mean-field dynamo • A large-scale seed + small-scale dynamo + Mean-field dynamo

  11. What says cosmology? • 1. Everything is known (this statement persists) • Nothing about homogeneous magnetic field • This idea looked strange 10 years ago • It looks attractive today • My interpretation: the topic is completely obscure

  12. A possibility to go further • Neronov and D.Semikoz: • Magnetic fields between galactic clusters • (10-15 G) • Faraday rotation? • Small-scale or large-scale fields?

More Related