Filter Results:
- Full text PDF available (24)
Publication Year
2006
2018
- This year (2)
- Last 5 years (16)
- Last 10 years (27)
Publication Type
Co-author
Journals and Conferences
Learn More
The properties of string networks at scales well below the horizon are poorly understood, but they enter critically into many observables. We argue that in some regimes, stretching will be the only… (More)
We use our model of the small scale structure on cosmic strings to develop further the result of Siemens, Olum, and Vilenkin that the gravitational radiation length scale on cosmic strings is smaller… (More)
We explore the integrability of five-dimensional minimal supergravity in the presence of three commuting Killing vectors. We argue that to see the integrability structure of the theory one… (More)
Using the inverse scattering method in six dimensions we construct the dipole black ring of five dimensional Einstein-Maxwell-dilaton theory with dilaton coupling a = 2 √ 2/3. The 5d theory can be… (More)
We investigate the thermodynamic equilibrium states of a rotating thin shell, i.e., a ring, in a (2+1)-dimensional spacetime with a negative cosmological constant. The inner and outer regions with… (More)
We extend our earlier model of the small scale structure of cosmic string networks through an improved treatment of the separation of long and short scales. We find that the production of small loops… (More)
- Jorge V. Rocha
- 2008
Large black holes in an asymptotically AdS spacetime have a dual description in terms of approximately thermal states in the boundary CFT. The reflecting boundary conditions of AdS prevent such black… (More)
- Jorge V. Rocha
- Physical review letters
- 2008
The equation governing the time evolution of the number density of loops in a cosmic string network is a detailed balance determined by energy conservation. We solve this equation with the inclusion… (More)
We construct exact, time-dependent, black hole solutions of Einstein-Maxwelldilaton theory with arbitrary dilaton coupling, a. For a = 1 this theory arises as the fourdimensional low-energy effective… (More)
We consider a population of small, high-velocity cosmic string loops. We assume the typical length of these loops is determined by the gravitational radiation scale and use the results of [1] which… (More)