Light superconducting strings in the galaxy

Francesc Ferrer, Tanmay Vachaspati

Research output: Chapter in Book/Report/Conference proceedingChapter

Abstract

Observations of the Milky Way by the SPI/INTEGRAL satellite have confirmed the presence of a strong 511 keV gamma ray line emission from the bulge, which requires an intense source of positrons in the galactic center. These observations are hard to account for by conventional astrophysical scenarios, whereas other proposals, such as light DM, face stringent constraints from the diffuse gamma ray background. Here we suggest that light superconducting strings could be the source of the observed 511 keV emission.The associated particle physics, at the ~ 1TeV scale, is within the reach of planned accelerator experiments, while the distinguishing spatial distribution, proportional to the galactic magnetic field, could be mapped by SPI or by future, more sensitive satellite missions.

Original languageEnglish (US)
Title of host publicationFrom Quantum to Cosmos: Fundamental Physics Research in Space
PublisherWorld Scientific Publishing Co.
Pages529-535
Number of pages7
ISBN (Print)9789814261210, 9814261203, 9789814261203
DOIs
StatePublished - Jan 1 2009
Externally publishedYes

Keywords

  • Galaxy
  • Positrons
  • Strings

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Fingerprint Dive into the research topics of 'Light superconducting strings in the galaxy'. Together they form a unique fingerprint.

  • Cite this

    Ferrer, F., & Vachaspati, T. (2009). Light superconducting strings in the galaxy. In From Quantum to Cosmos: Fundamental Physics Research in Space (pp. 529-535). World Scientific Publishing Co.. https://doi.org/10.1142/9789814261210_0043