Thermodynamics of graviton condensate and the Kiselev black hole
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Date
2020
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Abstract
In this thesis, we will present the thermodynamic study of a model that considers
the black hole as a condensation of gravitons (55) (56). We will obtain a correction to
the Hawking temperature and a negative pressure for a black hole of mass M. In this
way, the graviton condensate, which is assumed to be at the critical point defined by
the condition µch=0, will have well-defined thermodynamic quantities P, V , Th, S, and
U as any other Bose-Einstein condensate. We will also discuss the Kiselev black hole,
which has the capacity to parametrize the most well-known spherically symmetric black
holes. We will show that this is true, even at the thermodynamic level. Finally, we will
present a new metric, which we will call the BEC-Kiselev black hole, that will allow us
to extend the graviton condensate to the case of solutions with different types of the
energy-momentum tensor.In this thesis, we will present the thermodynamic study of a model that considers
the black hole as a condensation of gravitons (55) (56). We will obtain a correction to
the Hawking temperature and a negative pressure for a black hole of mass M. In this
way, the graviton condensate, which is assumed to be at the critical point defined by
the condition µch=0, will have well-defined thermodynamic quantities P, V , Th, S, and
U as any other Bose-Einstein condensate. We will also discuss the Kiselev black hole,
which has the capacity to parametrize the most well-known spherically symmetric black
holes. We will show that this is true, even at the thermodynamic level. Finally, we will
present a new metric, which we will call the BEC-Kiselev black hole, that will allow us
to extend the graviton condensate to the case of solutions with different types of the
energy-momentum tensor.In this thesis, we will present the thermodynamic study of a model that considers
the black hole as a condensation of gravitons (55) (56). We will obtain a correction to
the Hawking temperature and a negative pressure for a black hole of mass M. In this
way, the graviton condensate, which is assumed to be at the critical point defined by
the condition µch=0, will have well-defined thermodynamic quantities P, V , Th, S, and
U as any other Bose-Einstein condensate. We will also discuss the Kiselev black hole,
which has the capacity to parametrize the most well-known spherically symmetric black
holes. We will show that this is true, even at the thermodynamic level. Finally, we will
present a new metric, which we will call the BEC-Kiselev black hole, that will allow us
to extend the graviton condensate to the case of solutions with different types of the
energy-momentum tensor.In this thesis, we will present the thermodynamic study of a model that considers
the black hole as a condensation of gravitons (55) (56). We will obtain a correction to
the Hawking temperature and a negative pressure for a black hole of mass M. In this
way, the graviton condensate, which is assumed to be at the critical point defined by
the condition µch=0, will have well-defined thermodynamic quantities P, V , Th, S, and
U as any other Bose-Einstein condensate. We will also discuss the Kiselev black hole,
which has the capacity to parametrize the most well-known spherically symmetric black
holes. We will show that this is true, even at the thermodynamic level. Finally, we will
present a new metric, which we will call the BEC-Kiselev black hole, that will allow us
to extend the graviton condensate to the case of solutions with different types of the
energy-momentum tensor.In this thesis, we will present the thermodynamic study of a model that considers
the black hole as a condensation of gravitons (55) (56). We will obtain a correction to
the Hawking temperature and a negative pressure for a black hole of mass M. In this
way, the graviton condensate, which is assumed to be at the critical point defined by
the condition µch=0, will have well-defined thermodynamic quantities P, V , Th, S, and
U as any other Bose-Einstein condensate. We will also discuss the Kiselev black hole,
which has the capacity to parametrize the most well-known spherically symmetric black
holes. We will show that this is true, even at the thermodynamic level. Finally, we will
present a new metric, which we will call the BEC-Kiselev black hole, that will allow us
to extend the graviton condensate to the case of solutions with different types of the
energy-momentum tensor.In this thesis, we will present the thermodynamic study of a model that considers
the black hole as a condensation of gravitons (55) (56). We will obtain a correction to
the Hawking temperature and a negative pressure for a black hole of mass M. In this
way, the graviton condensate, which is assumed to be at the critical point defined by
the condition µch=0, will have well-defined thermodynamic quantities P, V , Th, S, and
U as any other Bose-Einstein condensate. We will also discuss the Kiselev black hole,
which has the capacity to parametrize the most well-known spherically symmetric black
holes. We will show that this is true, even at the thermodynamic level. Finally, we will
present a new metric, which we will call the BEC-Kiselev black hole, that will allow us
to extend the graviton condensate to the case of solutions with different types of the
energy-momentum tensor.In this thesis, we will present the thermodynamic study of a model that considers
the black hole as a condensation of gravitons (55) (56). We will obtain a correction to
the Hawking temperature and a negative pressure for a black hole of mass M. In this
way, the graviton condensate, which is assumed to be at the critical point defined by
the condition µch=0, will have well-defined thermodynamic quantities P, V , Th, S, and
U as any other Bose-Einstein condensate. We will also discuss the Kiselev black hole,
which has the capacity to parametrize the most well-known spherically symmetric black
holes. We will show that this is true, even at the thermodynamic level. Finally, we will
present a new metric, which we will call the BEC-Kiselev black hole, that will allow us
to extend the graviton condensate to the case of solutions with different types of the
energy-momentum tensor.In this thesis, we will present the thermodynamic study of a model that considers
the black hole as a condensation of gravitons (55) (56). We will obtain a correction to
the Hawking temperature and a negative pressure for a black hole of mass M. In this
way, the graviton condensate, which is assumed to be at the critical point defined by
the condition µch=0, will have well-defined thermodynamic quantities P, V , Th, S, and
U as any other Bose-Einstein condensate. We will also discuss the Kiselev black hole,
which has the capacity to parametrize the most well-known spherically symmetric black
holes. We will show that this is true, even at the thermodynamic level. Finally, we will
present a new metric, which we will call the BEC-Kiselev black hole, that will allow us
to extend the graviton condensate to the case of solutions with different types of the
energy-momentum tensor.In this thesis, we will present the thermodynamic study of a model that considers
the black hole as a condensation of gravitons (55) (56). We will obtain a correction to
the Hawking temperature and a negative pressure for a black hole of mass M. In this
way, the graviton condensate, which is assumed to be at the critical point defined by
the condition µch=0, will have well-defined thermodynamic quantities P, V , Th, S, and
U as any other Bose-Einstein condensate. We will also discuss the Kiselev black hole,
which has the capacity to parametrize the most well-known spherically symmetric black
holes. We will show that this is true, even at the thermodynamic level. Finally, we will
present a new metric, which we will call the BEC-Kiselev black hole, that will allow us
to extend the graviton condensate to the case of solutions with different types of the
energy-momentum tensor.In this thesis, we will present the thermodynamic study of a model that considers
the black hole as a condensation of gravitons (55) (56). We will obtain a correction to
the Hawking temperature and a negative pressure for a black hole of mass M. In this
way, the graviton condensate, which is assumed to be at the critical point defined by
the condition µch=0, will have well-defined thermodynamic quantities P, V , Th, S, and
U as any other Bose-Einstein condensate. We will also discuss the Kiselev black hole,
which has the capacity to parametrize the most well-known spherically symmetric black
holes. We will show that this is true, even at the thermodynamic level. Finally, we will
present a new metric, which we will call the BEC-Kiselev black hole, that will allow us
to extend the graviton condensate to the case of solutions with different types of the
energy-momentum tensor.
Description
Tesis (Master in Physics)--Pontificia Universidad Católica de Chile, 2020