Saved in:
| Main Authors: | , , , , , , , , , |
|---|---|
| Format: | Preprint |
| Published: |
2024
|
| Subjects: | |
| Online Access: | https://arxiv.org/abs/2405.00140 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866917654844932096 |
|---|---|
| author | Sirks, Ellen L. Harvey, David Massey, Richard Oman, Kyle A. Robertson, Andrew Frenk, Carlos Everett, Spencer Gill, Ajay S. Lagattuta, David McCleary, Jacqueline |
| author_facet | Sirks, Ellen L. Harvey, David Massey, Richard Oman, Kyle A. Robertson, Andrew Frenk, Carlos Everett, Spencer Gill, Ajay S. Lagattuta, David McCleary, Jacqueline |
| contents | Terrestrial particle accelerators collide charged particles, then watch the trajectory of outgoing debris - but they cannot manipulate dark matter. Fortunately, dark matter is the main component of galaxy clusters, which are continuously pulled together by gravity. We show that galaxy cluster mergers can be exploited as enormous, natural dark matter colliders. We analyse hydrodynamical simulations of a universe containing self-interacting dark matter (SIDM) in which all particles interact via gravity, and dark matter particles can also scatter off each other via a massive mediator. During cluster collisions, SIDM spreads out and lags behind cluster member galaxies. Individual systems can have quirky dynamics that makes them difficult to interpret. Statistically, however, we find that the mean or median of dark matter's spatial offset in many collisions can be robustly modelled, and is independent of our viewing angle and halo mass even in collisions between unequal-mass systems. If the SIDM cross-section were sigma/m = 0.1cm^2/g = 0.18 barn/GeV, the 'bulleticity' lag would be ~5 percent that of gas due to ram pressure, and could be detected at 95 percent confidence in weak lensing observations of ~100 well-chosen clusters. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2405_00140 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Hydrodynamical simulations of merging galaxy clusters: giant dark matter particle colliders, powered by gravity Sirks, Ellen L. Harvey, David Massey, Richard Oman, Kyle A. Robertson, Andrew Frenk, Carlos Everett, Spencer Gill, Ajay S. Lagattuta, David McCleary, Jacqueline Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology High Energy Physics - Theory Terrestrial particle accelerators collide charged particles, then watch the trajectory of outgoing debris - but they cannot manipulate dark matter. Fortunately, dark matter is the main component of galaxy clusters, which are continuously pulled together by gravity. We show that galaxy cluster mergers can be exploited as enormous, natural dark matter colliders. We analyse hydrodynamical simulations of a universe containing self-interacting dark matter (SIDM) in which all particles interact via gravity, and dark matter particles can also scatter off each other via a massive mediator. During cluster collisions, SIDM spreads out and lags behind cluster member galaxies. Individual systems can have quirky dynamics that makes them difficult to interpret. Statistically, however, we find that the mean or median of dark matter's spatial offset in many collisions can be robustly modelled, and is independent of our viewing angle and halo mass even in collisions between unequal-mass systems. If the SIDM cross-section were sigma/m = 0.1cm^2/g = 0.18 barn/GeV, the 'bulleticity' lag would be ~5 percent that of gas due to ram pressure, and could be detected at 95 percent confidence in weak lensing observations of ~100 well-chosen clusters. |
| title | Hydrodynamical simulations of merging galaxy clusters: giant dark matter particle colliders, powered by gravity |
| topic | Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology High Energy Physics - Theory |
| url | https://arxiv.org/abs/2405.00140 |