Searching for missing baryons through scintillation

Searching for missing baryons through scintillation

Cool molecular hydrogen H2 may be the ultimate possible constituent to the Milky-Way missing baryon. We describe a new way to search for such transparent matter in the Galactic disc and halo, through the diffractive and refractive effects on the light of background stars. By simulating the phase del...

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Bibliographic Details
Main Author: Habibi, Farhang
Language:ENG
Published: Université Paris Sud - Paris XI 2011
Subjects:
[PHYS:COND:CM_GEN] Physics/Condensed Matter/Other
Cosmology
Dark matter
Missing baryons
Disk
Halo
Structure
Local interstellar medium
ISM
molecular clouds
turbulence
Simulation
turbulent screen
Fresnel integral
FFT
Observation: ESO-NTT IR
SMC
dark nebulae
dust
Online Access:http://tel.archives-ouvertes.fr/tel-00625486
http://tel.archives-ouvertes.fr/docs/00/62/54/86/PDF/VD2_HABIBI_FARHANGH_15062011.pdf

Internet

http://tel.archives-ouvertes.fr/tel-00625486
http://tel.archives-ouvertes.fr/docs/00/62/54/86/PDF/VD2_HABIBI_FARHANGH_15062011.pdf

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