Permanent URL to this publication: http://dx.doi.org/10.5167/uzh-16533
Ripamonti, E; Mapelli, M; Zaroubi, S (2008). Radiation from early black holes – I. Effects on the neutral intergalactic medium. Monthly Notices of the Royal Astronomical Society, 387(1):158-172.
View at publisher
In the pre-reionization Universe, the regions of the intergalactic medium (IGM) which are far from luminous sources are the last to undergo reionization. Until then, they should be scarcely affected by stellar radiation; instead, the X-ray emission from an early black hole (BH) population can have much larger influence. We investigate the effects of such emission, looking at a number of BH model populations (differing for the cosmological density evolution of BHs, the BH properties, and the spectral energy distribution of the BH emission). We find that BH radiation can easily heat the IGM to 103–104 K , while achieving partial ionization. The most interesting consequence of this heating is that BHs are expected to induce a 21-cm signal ( δTb∼ 20–30 mK at z≲ 12 ) which should be observable with forthcoming experiments (e.g. LOFAR). We also find that at z≲ 10 BH emission strongly increases the critical mass separating star-forming and non-star-forming haloes.
17 downloads since deposited on 10 Mar 2009
3 downloads since 12 months
|Item Type:||Journal Article, refereed, original work|
|Communities & Collections:||07 Faculty of Science > Institute for Computational Science|
|Dewey Decimal Classification:||530 Physics|
|Deposited On:||10 Mar 2009 14:39|
|Last Modified:||16 Jan 2014 05:37|
|Additional Information:||The definitive version is available at www.blackwell-synergy.com|
Users (please log in): suggest update or correction for this item
Repository Staff Only: item control page