A possible challenge for cold and warm dark matter
Max Planck Institute for Astrophysics · University of Groningen · +8 more institutions
Abstract
Abstract Measuring the density profile and mass concentration of dark-matter haloes is a key test of the standard cold dark matter paradigm. Such objects are dark and thus challenging to characterize, but they can be studied via gravitational lensing. Recently, a million-solar-mass object was discovered superposed on an extended and extremely thin gravitational arc. Here we report on extensive tests of various assumptions for the mass density profile and redshift of this object. We find that models that best describe the data have two components: an unresolved point mass of radius ≤10 pc centred on an extended mass distribution with an almost constant surface density out to a truncation radius of 139 pc. These…
Citation impact
- FWCI
- 59.07
- Percentile
- 99%
- References
- 48
Authors
8- SVSimona VegettiCorresponding
Max Planck Institute for Astrophysics
- SDSimon D. M. White
Max Planck Institute for Astrophysics
- JPJohn P. McKean
University of Groningen, South African Radio Astronomy Observatory, University of Pretoria
- DPDevon Powell
Max Planck Institute for Astrophysics
- CSCristiana Spingola
Istituto di Radioastronomia di Bologna
Topics & keywords
- Dark matter
- Cold dark matter
- Dark matter halo
- Halo
- Mass distribution
- RADIUS
- Dark fluid
- Scalar field dark matter
Funding
- ECEuropean CommissionAwards: J33C22001170001, 758853, CN00000013, CUP J33C22001170001
- NRNational Research FoundationAward: 128943
- MDMinistero dell’Istruzione, dell’Università e della RicercaAwards: PNRR -M4C2, CN00000013
- MMax-Planck-Gesellschaft
- MDMinistero degli Affari Esteri e della Cooperazione InternazionaleAward: PGRZA23GR03
- H2Horizon 2020 Framework ProgrammeAward: 758853