Perturbations of global monopoles as a black hole’s hair
نویسندگان
چکیده
We study the stability of a spherically symmetric black hole with a global monopole hair. Asymptotically the spacetime is flat but has a deficit solid angle which depends on the vacuum expectation value of the scalar field. When the vacuum expectation value is larger than a certain critical value, this spacetime has a cosmological event horizon. We investigate the stability of these solutions against the spherical and polar perturbations and confirm that the global monopole hair is stable in both cases. Although we consider some particular modes in the polar case, our analysis suggests the conservation of the “topological charge” in the presence of the event horizons and violation of black hole no-hair conjecture in asymptotically non-flat spacetime. PACS numbers: 11.27.+d, 98.80.Cq 04.70.Bw Perturbations of global monopoles as a black hole’s hair 2
منابع مشابه
Perturbations of the global monopoles as a black hole’s hair
We study the stability of a spherically symmetric black hole with a global monopole hair. Asymptotically the spacetime is flat but has deficit solid angle which depends on the vacuum expectation value of the scalar field. When the vacuum expectation value is larger than a certain critical value, this spacetime has a cosmological event horizon. We investigate the stability of these solutions aga...
متن کاملGlobal monopoles, cosmological constant and maximal mass conjecture
We consider global monopoles as well as black holes with global monopole hair in Einstein-Goldstone model with a cosmological constant in four spacetime dimensions. Similar to the Λ = 0 case, the mass of these solutions defined in the standard way diverges. We use a boundary counterterm subtraction method to compute the mass and action of Λ 6= 0 configurations. The mass of the asymptotically de...
متن کاملGravitational axial perturbations and quasinormal modes of loop quantum black holes
Gravitational waves can be used as a way to investigate the structure of spacetime. Loop Quantum Gravity is a theory that propose a way to model the behavior of spacetime in situations where its atomic characteristic arises. Among these situations, the spacetime behavior near the Big Bang or black hole’s singularity. A recent prediction of loop quantum gravity is the existence of sub-Planckian ...
متن کاملRotating Black Holes with Monopole Hair
We study rotating black holes in Einstein-Yang-Mills-Higgs theory. These black holes emerge from static black holes with monopole hair when a finite horizon angular velocity is imposed. At critical values of the horizon angular velocity and the horizon radius, they bifurcate with embedded Kerr-Newman black holes. The non-Abelian black holes possess an electric dipole moment, but no electric cha...
متن کاملBlack Holes with Zero Mass
We consider the spacetimes corresponding to static Global Monopoles with interior boundaries corresponding to a Black Hole Horizon and analyze the behavior of the appropriate ADM mass as a function of the horizon radius rH . We find that for small enough rH , this mass is negative as in the case of the regular global monopoles, but that for large enough rH the mass becomes positive encountering...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2004