PoS - Proceedings of Science
Volume 454 - 1st General Meeting and 1st Training School of the COST Action COSMIC WSIPers (COSMICWISPers) - Traning School Talks
Constraining Ultra-Light Scalar Dark Matter with Pulsars
P. Kus*, D.L. Nacir and F. Urban
Full text: Not available
Abstract
Binary pulsars can serve as natural dark matter detectors. We consider an ultralight scalar dark matter, which interacts directly with the binary pulsar components via a universal effective interaction, characterized by one coupling constant. This causes a perturbation of the dynamics of the binary system. The perturbation is manifested by a change in the arrival time of pulses from the pulsar on Earth. The aim of our work is to determine the limiting value of the coupling constant, enabling the measurement of this effect. In other words, time residuals can serve as a proxy for ULDM. In this proceedings, a simple approach to sensitivity curve construction (i.e., a plot of the coupling constant versus particle mass) is presented. Further details and a comprehensive analysis can be found in [1].
How to cite

Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.