Self-similar solutions for fuzzy dark matter
Raquel Galazo-Garcia, Philippe Brax, Patrick Valageas
SciPost Phys. Proc. 12, 060 (2023) · published 5 July 2023
- doi: 10.21468/SciPostPhysProc.12.060
- Submissions/Reports
Proceedings event
14th International Conference on Identification of Dark Matter
Abstract
Self-similar solutions for fuzzy dark matter are very different from their counterparts in the standard cold dark matter model. In contrast to the familiar hierarchical collapse of the current model for structure formation, they correspond to an inverse hierarchical blow-up. This fact highlights the gravitational cooling process, which in the absence of dissipation, allows the system to eject excess energy through the intermittent expulsion of clumps of matter. These surprising behaviours are due to the wave properties of the Schrödinger equation and to the quantum pressure. These features are printed in the Eulerian density-velocity representation of the nonrelativistic scalar field, or in the Lagrangian representation in the mass-shell trajectories.
Authors / Affiliations: mappings to Contributors and Organizations
See all Organizations.- 1 Raquel Galazo-Garcia,
- 1 2 Philippe Brax,
- 1 Patrick Valageas
- 1 Université Paris-Saclay / University of Paris-Saclay
- 2 Organisation européenne pour la recherche nucléaire / European Organization for Nuclear Research [CERN]
- Agence Nationale de la Recherche [ANR]
- Commissariat à l'Énergie Atomique et aux Énergies Alternatives (through Organization: Commissariat à l'énergie Atomique et aux énergies Alternatives / Atomic Energy and Alternative Energies Commission [CEA])
- Horizon 2020 (through Organization: European Commission [EC])
- Institut National de Physique Nucléaire et de Physique des Particules [IN2P3]
- Université Paris-Saclay / University of Paris-Saclay