46 pages, 1 figure, LaTeXInternational audienceWe construct the first explicit, smooth, horizonless black-hole microstate geometry whose moduli space is described by an arbitrary function of one variable and is thus infinite-dimensional. This is achieved by constructing the scalar Green function on a simple D6 anti-D6 background, and using this Green function to obtain the fully back-reacted solution for a supertube with varying charge density in this background. We show that this supertube can store parametrically more entropy than in flat space, confirming the entropy enhancement mechanism that was predicted using brane probes. We also show that all the local properties of the fully back-reacted solution can, in fact, be obtained using th...
v2: reference added. journal versionInternational audienceWe argue that there exists a new class of ...
2014-06-10In this thesis we explore two novel directions in the quest for 3-charge ""black hole micr...
If one encodes the gravitational degrees of freedom in an orthonormal frame field there is a very na...
46 pages, 1 figure, LaTeXInternational audienceWe construct the first explicit, smooth, horizonless ...
2018-07-26In this thesis we investigate different aspects of supersymmetric microstate geometries an...
UnrestrictedIn this thesis, we discuss the possibility of exploring the statistical mechanics descri...
2015-06-19In this thesis we examine smooth supergravity solutions known as ""microstate geometries""...
All known horizonless black-hole microstate geometries correspond to brane sources that acquire a fi...
There are, by now, several arguments that superstrata, which represent D1-D5-P bound states that dep...
25 pages, 9 figuresInternational audienceWe study the dynamics of supertubes in smooth bubbling geom...
There are, by now, several arguments that superstrata, which represent D1-D5-P bound states that dep...
35 pages, 3 figuresInternational audienceThere are, by now, several arguments that superstrata, whic...
We review the thermodynamic behaviour and paradoxes arising from a classical description of Black Ho...
We propose that every supersymmetric four dimensional black hole of finite area can be split up into...
We argue that there exists a new class of completely smooth 1/8-BPS, three-charge bound state config...
v2: reference added. journal versionInternational audienceWe argue that there exists a new class of ...
2014-06-10In this thesis we explore two novel directions in the quest for 3-charge ""black hole micr...
If one encodes the gravitational degrees of freedom in an orthonormal frame field there is a very na...
46 pages, 1 figure, LaTeXInternational audienceWe construct the first explicit, smooth, horizonless ...
2018-07-26In this thesis we investigate different aspects of supersymmetric microstate geometries an...
UnrestrictedIn this thesis, we discuss the possibility of exploring the statistical mechanics descri...
2015-06-19In this thesis we examine smooth supergravity solutions known as ""microstate geometries""...
All known horizonless black-hole microstate geometries correspond to brane sources that acquire a fi...
There are, by now, several arguments that superstrata, which represent D1-D5-P bound states that dep...
25 pages, 9 figuresInternational audienceWe study the dynamics of supertubes in smooth bubbling geom...
There are, by now, several arguments that superstrata, which represent D1-D5-P bound states that dep...
35 pages, 3 figuresInternational audienceThere are, by now, several arguments that superstrata, whic...
We review the thermodynamic behaviour and paradoxes arising from a classical description of Black Ho...
We propose that every supersymmetric four dimensional black hole of finite area can be split up into...
We argue that there exists a new class of completely smooth 1/8-BPS, three-charge bound state config...
v2: reference added. journal versionInternational audienceWe argue that there exists a new class of ...
2014-06-10In this thesis we explore two novel directions in the quest for 3-charge ""black hole micr...
If one encodes the gravitational degrees of freedom in an orthonormal frame field there is a very na...