IIA Institutional Repository

The Problem of a Primordial Black Hole Hydrogenlike Atom

Show simple item record

dc.contributor.author de Sabbata, V
dc.contributor.author Sivaram, C
dc.date.accessioned 2008-10-24T14:31:56Z
dc.date.available 2008-10-24T14:31:56Z
dc.date.issued 1994-03
dc.identifier.citation Physics Essays, Vol. 7, No. 1, pp. 103 - 106 en
dc.identifier.issn 0836-1398
dc.identifier.uri http://hdl.handle.net/2248/3965
dc.description.abstract It is shown that the recently proposed system composed of an electron and a primordial black hole forming a hydrogenlike atomic system cannot be stable, because the radiation pressure acting on the electron from Hawking radiation of the black hole far exceeds the binding force. On the contrary, if the black hole has a zero Hawking temperature, either due to its charge or spin, the required values of these parameters are so large that the electron would still not be stably bound to the black hole. However, if the black hole has a magnetic moment due to its spin, then electrons passing by the black hole could have spin-flip transitions producing high-energy gamma rays of ~1014 eV − 1015 eV.
dc.language.iso en en
dc.publisher Physics Essays Publication en
dc.relation.uri http://dx.doi.org/10.4006/1.3029104 en
dc.title The Problem of a Primordial Black Hole Hydrogenlike Atom en
dc.type Article en


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search DSpace


Browse

My Account