Renormalization Group Flows for Quantum Gravity
... Renormalization Group Flows for Quantum Gravity ...
... Renormalization Group Flows for Quantum Gravity ...
General Relativity Needs No Interpretation
... for it in this sense.4 Let us say, then, that we have a framework some aspect of the semantic structure of which is, for one reason or another, poorly understood. One natural route of attack in the attempt to grasp it better is to try to find another framework that we do understand, in the terms of ...
... for it in this sense.4 Let us say, then, that we have a framework some aspect of the semantic structure of which is, for one reason or another, poorly understood. One natural route of attack in the attempt to grasp it better is to try to find another framework that we do understand, in the terms of ...
Phase Transitions in Early Universe
... In the past few decades, people’s knowledge on the universe and the elementary particles has boosted a lot. In the cosmology, many interesting and puzzling results have enriched our understanding about the universe while we have been trying to unveil its origin and future since early human history. ...
... In the past few decades, people’s knowledge on the universe and the elementary particles has boosted a lot. In the cosmology, many interesting and puzzling results have enriched our understanding about the universe while we have been trying to unveil its origin and future since early human history. ...
Phys. Rev. Lett. 105 - Physics (APS)
... Bi2 Se3 [12], Bi2 Te3 [13], and Sb2 Te3 [14] consist of a single massless Dirac cone [9]. Crossing of the two surface state branches with opposite spins in the materials is fully protected by the time-reversal (TR) symmetry at the Dirac points, which cannot be destroyed by any TR invariant perturbat ...
... Bi2 Se3 [12], Bi2 Te3 [13], and Sb2 Te3 [14] consist of a single massless Dirac cone [9]. Crossing of the two surface state branches with opposite spins in the materials is fully protected by the time-reversal (TR) symmetry at the Dirac points, which cannot be destroyed by any TR invariant perturbat ...
Axiomatic description of mixed states from Selinger`s CPM
... A,B (f : C ⊗ A → C ⊗ B) := λ†B ◦ (p1Cq ⊗ 1B )† ◦ (1C ∗ ⊗ f ) ◦ (p1Cq ⊗ 1A ) ◦ λA : A → B , play a crucial role in quantum information theory. To our knowledge, the need for an abstract notion of internal trace has so far only been indicated by Delbecque in [5], motivated by the fact that while in Se ...
... A,B (f : C ⊗ A → C ⊗ B) := λ†B ◦ (p1Cq ⊗ 1B )† ◦ (1C ∗ ⊗ f ) ◦ (p1Cq ⊗ 1A ) ◦ λA : A → B , play a crucial role in quantum information theory. To our knowledge, the need for an abstract notion of internal trace has so far only been indicated by Delbecque in [5], motivated by the fact that while in Se ...
The general structure of quantum resource theories
... Note that clearly free operations can convert one resource state into another. The intuition is that free operations can not convert a resource state into a more resourceful state. However, the term “more” resourceful implies a total order or hierarchy of resources. Such a total order does not exist ...
... Note that clearly free operations can convert one resource state into another. The intuition is that free operations can not convert a resource state into a more resourceful state. However, the term “more” resourceful implies a total order or hierarchy of resources. Such a total order does not exist ...
On principles of repulsive gravity: the Elementary Process Theory
... the experimental physicists involved in the aforementioned projects are driven by curiosity rather than by a belief in repulsive gravity. In the literature several theoretical arguments against repulsive gravity can be found; these, however, lean on assumptions that include the validity of contempor ...
... the experimental physicists involved in the aforementioned projects are driven by curiosity rather than by a belief in repulsive gravity. In the literature several theoretical arguments against repulsive gravity can be found; these, however, lean on assumptions that include the validity of contempor ...
a ∇ µ
... differs from the distribution matter density for Coulomb solution. Thus the proposed idea is that some galaxies are immersed in a cloud of a classical gauge field. The SU(3) classical gauge field does not interact with ordinary matter because ordinary matter is colorless. Thus one can suppose that SU ...
... differs from the distribution matter density for Coulomb solution. Thus the proposed idea is that some galaxies are immersed in a cloud of a classical gauge field. The SU(3) classical gauge field does not interact with ordinary matter because ordinary matter is colorless. Thus one can suppose that SU ...
Establish analytical and numerical theory of light emission
... correct description treatment of the problem. The collective emission by a cloud of atoms is described fully quantum mechanically, and the quantum field emitted by each atom is propagating and hence affects all other atoms in the sample. Our previous attempts on this problem, dealt with i) a scalar ...
... correct description treatment of the problem. The collective emission by a cloud of atoms is described fully quantum mechanically, and the quantum field emitted by each atom is propagating and hence affects all other atoms in the sample. Our previous attempts on this problem, dealt with i) a scalar ...
PDF
... vector space Rk via φ, and the set |K| inherits a metric from Rk making it into a metric space and topological space. The isometry class of K is independent of the choice of the bijection φ. Examples: ∗ hSimplicialComplexi created: h2013-03-21i by: hdjaoi version: h32828i Privacy setting: h1i hDefin ...
... vector space Rk via φ, and the set |K| inherits a metric from Rk making it into a metric space and topological space. The isometry class of K is independent of the choice of the bijection φ. Examples: ∗ hSimplicialComplexi created: h2013-03-21i by: hdjaoi version: h32828i Privacy setting: h1i hDefin ...
Gravitational Repulsion within a Black-Hole
... coinciding with the Newtonian world time, accounting for classical as well as quantum relativistic evolution. The world time τ provides a parameter that labels the dynamical evolution of the covariant system. For free on shell motion of a single particle, the Einstein proper time can be taken equal ...
... coinciding with the Newtonian world time, accounting for classical as well as quantum relativistic evolution. The world time τ provides a parameter that labels the dynamical evolution of the covariant system. For free on shell motion of a single particle, the Einstein proper time can be taken equal ...