| 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. |
| Přispěvatelé: |
Foundation for Research and Technology - Hellas, California Institute of Technology, University of Manchester, Metsähovi Radio Observatory, University of Groningen, Max-Planck-Institut für Radioastronomie, University of Crete, Aalto-yliopisto, Aalto University |
| Jazyk: |
angličtina |
| Rok vydání: |
2021 |
| Předmět: |
|
| Popis: |
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 their gravitational effect on distant sources. The same applies to primordial black holes, considered as an alternative scenario to DM particle models. However, there is still no evidence for the existence of such objects. With the aim of finding compact objects in the mass range of ∼106-109 M·, we search for strong gravitational lenses on milliarcsec scales ( |
| Databáze: |
OpenAIRE |
| Externí odkaz: |
|
