Journal
PHYSICAL REVIEW LETTERS
Volume 126, Issue 4, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.126.041105
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Funding
- Paper Enhancement Grant at the University of Nottingham
- Royal Society [UF120112]
- Royal Society Enhancement Grant [RGF/EA/180286]
- EPSRC [EP/P00637X/1]
- STFC [ST/P000703]
- [A2RHS2]
- Royal Society [UF120112] Funding Source: Royal Society
- EPSRC [EP/P00637X/1] Funding Source: UKRI
- STFC [ST/S002227/1] Funding Source: UKRI
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Research has shown that fluid mechanical analogue black hole systems exhibit significant global mass changes in the presence of waves, leading to the possibility of studying backreaction with the presence of a dynamical metric.
Analogue models of gravity, particularly fluid mechanical analogues, have been very successful in mimicking the behavior of fields around black holes. However, hydrodynamic black holes are externally driven systems whose effective mass and angular momentum arc set by experimental parameters, and, as such, no appreciable internal backreaction is expected to take place. On the contrary, we show using a rotating draining vortex flow that a fluid system of finite size responds to the presence of waves on timescales much longer than the wave dynamics, which leads to a significant global change in the total mass of our system. This backreaction is encapsulated by a dynamical metric, raising the possibility of studying backreaction in analogue black hole spacetimes.
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