SMILE

Autor: M. Mastorakis, Konstantinos Tassis, Ian Browne, K. E. Dolapsaki, A. C. S. Readhead, P. N. Wilkinson, Carolina Casadio, Vincent Pelgrims, V. Diamantopoulos, G. Kalaitzidakis, K. Psarras, Talvikki Hovatta, Vasiliki Pavlidou, K. Gkimisi, H. K. Vedantham, J. A. Zensus, D. Blinov, Evangelia Ntormousi, K. Nikolaou, N. Mandarakas

Publikováno v: Monthly Notices of the Royal Astronomical Society, 507(1), L6-L10
Monthly Notices of the Royal Astronomical Society, 507, L6-L10. Oxford University Press

Dark Matter (DM) halos with masses below $\sim10^{8}$ $M_{\odot}$, which would help to discriminate between DM models, may be detected through their gravitational effect on distant sources. The same applies to primordial black holes, considered as an

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2a07ec66cc7e430d47e9ee2cb70523d9
https://doi.org/10.1093/mnrasl/slab082

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