2017
DOI: 10.1007/jhep09(2017)048
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Quasi-normal modes from non-commutative matrix dynamics

Abstract: Abstract:We explore similarities between the process of relaxation in the BMN matrix model and the physics of black holes in AdS/CFT. Focusing on Dyson-fluid solutions of the matrix model, we perform numerical simulations of the real time dynamics of the system. By quenching the equilibrium distribution we study quasi-normal oscillations of scalar single trace observables, we isolate the lowest quasi-normal mode, and we determine its frequencies as function of the energy. Considering the BMN matrix model as a … Show more

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Cited by 4 publications
(5 citation statements)
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References 39 publications
(88 reference statements)
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“…The behavior of ν seems to be smooth and continuous with energy, and as such is apparently insensitive to the phase change near (2.14). Furthermore, our results for ν are consistent with those from matrix model simulations which do not suffer from UV problems [59], to which our simulations reduce to in the zero volume limit.…”
Section: Possible Observation Of Quasinormal Modessupporting
confidence: 89%
“…The behavior of ν seems to be smooth and continuous with energy, and as such is apparently insensitive to the phase change near (2.14). Furthermore, our results for ν are consistent with those from matrix model simulations which do not suffer from UV problems [59], to which our simulations reduce to in the zero volume limit.…”
Section: Possible Observation Of Quasinormal Modessupporting
confidence: 89%
“…Finally, let us note that at high temperatures we can use equations ( 30), ( 31), ( 25) and ( 23) to estimate the real part of the quasinormal frequency of the quasinormal ringing of Tr X 2 i as w XX = 4.89 T 1/4 , which agrees well with the dependence w XX = 5.152 T 1/4 obtained in [62,71] for the bosonic matrix model using more elaborate dedicated simulations. At the highest temperatures where Im (w X ) can still be estimated in our simulations, we obtain Im (w X ) /Re (w X ) ∼ 0.1, which also roughly agrees with the result of [62,71]. According to the dual gravity calculation, near zero temperature the quasinormal frequency is proportional to T and the ratio Im (w X ) /Re (w X ) is about 1.7 [72].…”
Section: And Estimatesupporting
confidence: 84%
“…Due to its chaoticity and ergodicity, classical matrix mechanics exhibits real-time thermalization towards a dynamical equilibrium state in which long-time averages of physical observables approach their thermal equilibrium values [27]. This thermalization process can be also interpreted as quasinormal ringing characterized by nontrivial complex-valued quasinormal frequencies [61,62], with real parts being quite close to our estimates (30) and (31), see Subsection V C.…”
Section: A Bosonic Matrix Modelsupporting
confidence: 82%
“…The master fields should be related to classical geometry, when the theory admits a weakly-curved gravity dual. Previously, the classical dynamics of the Yang-Mills matrix model has been studied [39][40][41][42][43] with the expectation that typical configurations in the classical theory capture the aspects of the gravitational geometry. Therefore, the specific properties of the master field discussed in this paper should have some geometric interpretation.…”
Section: Conclusion and Discussionmentioning
confidence: 99%