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pro vyhledávání: '"Dolapsaki, K E"'
Autor:
Casadio, C., Blinov, D., Readhead, A. C. S., Browne, I. W. A., Wilkinson, P. N., Hovatta, T., Mandarakas, N., Pavlidou, V., Tassis, K., Vedantham, H. K., Zensus, J. A., Diamantopoulos, V., Dolapsaki, K. E., Gkimisi, K., Kalaitzidakis, G., Mastorakis, M., Nikolaou, K., Ntormousi, E., Pelgrims, V., Psarras, K.
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:
http://arxiv.org/abs/2107.06896
Autor:
Casadio, C., Blinov, D., Readhead, A.C.S., Browne, I.W.A., Wilkinson, P. N., Hovatta, T., Mandarakas, N., Pavlidou, V., Tassis, K., Vedantham, H. K., Zensus, J. A., Diamantopoulos, V., Dolapsaki, K. E., Gkimisi, K., Kalaitzidakis, G., Mastorakis, M., Nikolaou, K., Ntormousi, E., Pelgrims, V., Psarras, K.
Publisher Copyright: © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society. Dark matter (DM) haloes with masses below ∼108 M·, which would help to discriminate between DM models, may be detected through
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______661::de579a839eb41a6db09a37090a1b4051
https://aaltodoc.aalto.fi/handle/123456789/110094
https://aaltodoc.aalto.fi/handle/123456789/110094
Autor:
Casadio, C, Blinov, D, Readhead, A C S, Browne, I W A, Wilkinson, P N, Hovatta, T, Mandarakas, N, Pavlidou, V, Tassis, K, Vedantham, H K, Zensus, J A, Diamantopoulos, V, Dolapsaki, K E, Gkimisi, K, Kalaitzidakis, G, Mastorakis, M, Nikolaou, K, Ntormousi, E, Pelgrims, V, Psarras, K
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters; Oct2021, Vol. 507 Issue 1, pL6-L10, 5p
