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Multimachine stability analysis is crucial for understanding the dynamics and stability of power systems with multiple synchronous machines. The objective is to solve the swing equations for a network of M machines connected to an N-bus power system.
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Understanding the stability of equilibrium configurations is a fundamental part of mechanical engineering. In any system, there are three distinct types of equilibrium: stable, neutral, and unstable.
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Magnetically Induced Rotating Rayleigh-Taylor Instability
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Evolution and End Point of the Black String Instability: Large D Solution.

Roberto Emparan1,2, Ryotaku Suzuki3, Kentaro Tanabe4

  • 1Institució Catalana de Recerca i Estudis Avançats (ICREA) Passeig Lluís Companys 23, E-08010 Barcelona, Spain.

Physical Review Letters
|September 16, 2015
PubMed
Summary
This summary is machine-generated.

Thin black strings are unstable and evolve into stable, nonuniform configurations. This instability leads to periodic arrays of black holes in higher dimensions, confirming theoretical predictions.

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Area of Science:

  • Theoretical physics
  • String theory
  • General relativity

Background:

  • Black strings and branes are theoretical objects in higher-dimensional spacetimes.
  • Understanding their stability and evolution is crucial for string theory and quantum gravity.
  • Previous conjectures suggested instabilities in black strings at large dimensions.

Purpose of the Study:

  • To derive and solve nonlinear partial differential equations for black string and brane dynamics.
  • To investigate the stability of black strings in the large-D expansion.
  • To confirm theoretical predictions about the endpoint of black string instabilities.

Main Methods:

  • Derivation of (1+1)-dimensional nonlinear partial differential equations.
  • Numerical solutions to these equations.
  • Analysis of the dynamical evolution of black strings and branes.

Main Results:

  • Thin black strings are unstable to developing inhomogeneities.
  • Unstable black strings asymptote to stable, nonuniform configurations.
  • Very thin initial strings form periodic arrays of black holes connected by necks.
  • Equations for anti-de Sitter black brane dynamics at large D are presented.

Conclusions:

  • The study confirms the conjecture on black string instability endpoints in large dimensions.
  • Nonlinear dynamics lead to stable, nonuniform black string states.
  • The findings provide insights into the behavior of black objects in higher dimensions.