------------------------------------------------------------------------ galpos.tex PRL, Aug 2006, in press Date: Wed, 16 Aug 2006 17:33:25 -0400 To: gcnews@aoc.nrao.edu X-Mailer: Apple Mail (2.624) X-Virus-Scanned: ClamAV 0.88.4/1662/Tue Aug 15 04:29:25 2006 on delos.mps.ohio-state.edu X-Virus-Status: Clean X-MailScanner-Information: Please contact postmaster@aoc.nrao.edu for more information X-MailScanner: Found to be clean X-MailScanner-SpamCheck: not spam, SpamAssassin (score=0, required 5, autolearn=disabled) X-MailScanner-From: beacom@mps.ohio-state.edu X-Spam-Status: No % astro-ph/0512411 \documentclass[ aps, % American Physical Society prl, % Physical Review Letters showpacs, % Displays PACS after abstract superscriptaddress, % Authors' addresses linked with superscripts nofootinbib, % Does not treat footnotes as references twocolumn, % floatfix, nobalancelastpage]{revtex4} \usepackage{graphicx} \usepackage{epstopdf} \usepackage{natbib} \linespread {0.97} \begin{document} %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% \title{\large Stringent Constraint on Galactic Positron Production % Making Milky Way Positrons Without Artificial Ingredients \normalsize} \author{John F. Beacom} %\email{beacom@mps.ohio-state.edu} \affiliation{Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA} \affiliation{Department of Astronomy, The Ohio State University, Columbus, Ohio 43210, USA} \author{Hasan Y{\"u}ksel} %\email{yuksel@mps.ohio-state.edu} \affiliation{Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA} \date{15 December 2005; minor revisions, 24 July 2006} \begin{abstract} The intense 0.511 MeV gamma-ray line emission from the Galactic Center observed by INTEGRAL requires a large annihilation rate of nonrelativistic positrons. If these positrons are injected at even mildly relativistic energies, higher-energy gamma rays will also be produced. We calculate the gamma-ray spectrum due to inflight annihilation and compare to the observed diffuse Galactic gamma-ray data. Even in a simplified but conservative treatment, we find that the positron injection energies must be $\lesssim 3$ MeV, which strongly constrains models for Galactic positron production. \end{abstract} -- ---------------------------------------------------------------------- John Beacom Assistant Professor Department of Physics and Department of Astronomy Ohio State University email: beacom@mps.ohio-state.edu phone: (614) 247 - 8102 fax: (614) 292 - 7557 Dept. of Physics, OSU, 191 W. Woodruff Ave., Columbus, OH 43210 ----------------------------------------------------------------------