2016
DOI: 10.1209/0295-5075/114/60011
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Numerical study of a recent black-hole lasing experiment

Abstract: We theoretically analyse a recent experiment reporting the observation of a self-amplifying Hawking radiation in a flowing atomic condensate [1]. We are able to accurately reproduce the experimental observations using a theoretical model based on the numerical solution of a mean-field Gross-Pitaevskii equation that does not include quantum fluctuations of the matter field. In addition to confirming the black hole lasing mechanism, our results show that the underlying dynamical instability has a classical hydro… Show more

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Cited by 38 publications
(82 citation statements)
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“…This is similar to the pattern we have seen induced by number fluctuations on the WH side of the cavity, but not on the BH side. It should also be noted that the step potential fluctuations introduced in [6] were more than two orders of magnitude larger than in the experiment [8], whereas the number fluctuations we have introduced are comparable to those encountered in BEC experiments. Ref.…”
Section: Comparison With Other Simulated Resultssupporting
confidence: 60%
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“…This is similar to the pattern we have seen induced by number fluctuations on the WH side of the cavity, but not on the BH side. It should also be noted that the step potential fluctuations introduced in [6] were more than two orders of magnitude larger than in the experiment [8], whereas the number fluctuations we have introduced are comparable to those encountered in BEC experiments. Ref.…”
Section: Comparison With Other Simulated Resultssupporting
confidence: 60%
“…a zero frequency standing wave arises in the cavity, extending from the WH to the BH [6][7][8], as shown in Fig. 1(a-d) and Fig.…”
mentioning
confidence: 91%
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“…The previous equation has been shown to describe quite well the effective 1D dynamics of a trapped condensate in a wide range of situations [22,65]. Due to the chosen normalization, n(x, t) = |ψ(x, t)| 2 is the 1D density…”
Section: B Time-dependent Scenariosmentioning
confidence: 90%
“…In addition, there should not be substantial differences in the linear regime with respect to the usual flat-profile BHL. Moreover, thinking in a realistic implementation, the computed stationary solutions should still govern the late time dynamics once the system enters into the non-linear regime [27,29] regardless of the specific mechanism giving rise to the initial growth of the instability at short times [32][33][34].…”
Section: General Relation Between Black Holes and Black-hole Lasersmentioning
confidence: 99%