e - Instituto de Física Facultad de Ciencias
... Up to know, the EM field has no dynamics. This is introduced in a natural way by the gauge invariant field EM tensor ...
... Up to know, the EM field has no dynamics. This is introduced in a natural way by the gauge invariant field EM tensor ...
Some remarks on the Quantum Hall Effect - IPhT
... This partition function was computed exactly for m = 1 in [17] with orthogonal polynomials (in section (5) these polynomials will be described explicitly). Here, in order to illustrate the emergence of the edge physics we look at it from a semi-classical point of view and limit ourselves to t << 1. ...
... This partition function was computed exactly for m = 1 in [17] with orthogonal polynomials (in section (5) these polynomials will be described explicitly). Here, in order to illustrate the emergence of the edge physics we look at it from a semi-classical point of view and limit ourselves to t << 1. ...
1 Applying Quantum Optimization Algorithms for Linear Programming
... allows one to efficiently determine whether two sets of linear equations have the same solution [3], as well as many other simple global properties [4]. The HHL algorithm is likely to find applications in settings where the matrix A and the vector b are generated algorithmically, rather than being w ...
... allows one to efficiently determine whether two sets of linear equations have the same solution [3], as well as many other simple global properties [4]. The HHL algorithm is likely to find applications in settings where the matrix A and the vector b are generated algorithmically, rather than being w ...
Gravity and dark energy from quantum information
... 3) Zero Cosmological Constant and Nonzero Dark Energy from Holographic ...
... 3) Zero Cosmological Constant and Nonzero Dark Energy from Holographic ...
Gonzalez-MestresPreBigBang
... => Lorentz-like metrics can be naturally stable metric configurations for matter, spontaneoulsy generated from other initial metrics => relativity can be a (composite) expression of this phenomenon. The spinorial space-time just described has a t = 0 (ξ = 0) point where the Universe is supposed to b ...
... => Lorentz-like metrics can be naturally stable metric configurations for matter, spontaneoulsy generated from other initial metrics => relativity can be a (composite) expression of this phenomenon. The spinorial space-time just described has a t = 0 (ξ = 0) point where the Universe is supposed to b ...
Carbon – Science and Technology
... arrmchair GNRs. It is well known that the above problems provide a drop of the carrier mobility in graphene, thus limiting the device performance (e.g. field effect transistor cut-off frequency). In Figure (3), we calculate the S-parameters of a GNR with periodic vacancy, or in the presence of spuri ...
... arrmchair GNRs. It is well known that the above problems provide a drop of the carrier mobility in graphene, thus limiting the device performance (e.g. field effect transistor cut-off frequency). In Figure (3), we calculate the S-parameters of a GNR with periodic vacancy, or in the presence of spuri ...
Document
... Masses higher than 1700 MeV, width ~ hundreds MeV Mass of the pentaquark is roughly 5 M +(strangeness) ~ 1800 MeV An additional q –anti-q pair is added as constituent ...
... Masses higher than 1700 MeV, width ~ hundreds MeV Mass of the pentaquark is roughly 5 M +(strangeness) ~ 1800 MeV An additional q –anti-q pair is added as constituent ...
Aalborg Universitet
... delta potentials either all repulsive or all attractive, but rather few papers deal with the mixed case. We mention the work of Rosenthal, [7], where he considered M = ∞. The aim of this paper is to make a systematic mathematical study of the Rosenthal results and extend them to the case M < ∞. It h ...
... delta potentials either all repulsive or all attractive, but rather few papers deal with the mixed case. We mention the work of Rosenthal, [7], where he considered M = ∞. The aim of this paper is to make a systematic mathematical study of the Rosenthal results and extend them to the case M < ∞. It h ...
Einstein-Rosen Bridge (ER), Einstein-Podolsky
... 3. What Is a Wormhole from the View Point of Measure Theory? It is almost a trivial conclusion that a wormhole [7]-[31] is the quintessential empty set with varying degrees of emptiness corresponding to varying degrees of entanglement [1] [37] [45]. Our spacetime consists exclusively of zero sets qu ...
... 3. What Is a Wormhole from the View Point of Measure Theory? It is almost a trivial conclusion that a wormhole [7]-[31] is the quintessential empty set with varying degrees of emptiness corresponding to varying degrees of entanglement [1] [37] [45]. Our spacetime consists exclusively of zero sets qu ...
Magneto-optical properties of charged excitons in quantum dots
... model system for the investigation of quantum mechanical electron-electron interactions. This is because Coulomb blockade allows electrons to be added or removed one by one simply with a gate electrode.1,2 As a result, the electrical,2 optical,3– 6 and magnetic properties7 are tunable. An exciton co ...
... model system for the investigation of quantum mechanical electron-electron interactions. This is because Coulomb blockade allows electrons to be added or removed one by one simply with a gate electrode.1,2 As a result, the electrical,2 optical,3– 6 and magnetic properties7 are tunable. An exciton co ...
Existence Theorems in the Geometrically Non-linear 6
... been investigated using a variety of methods, such as the method of formal asymptotic expansions or the Γ -convergence analysis, see, e.g., [1, 2, 21, 34, 35, 39–41]. For an extensive treatment of this topic, as well as many bibliographic references, we refer to the books of Ciarlet [12, 13]. To the ...
... been investigated using a variety of methods, such as the method of formal asymptotic expansions or the Γ -convergence analysis, see, e.g., [1, 2, 21, 34, 35, 39–41]. For an extensive treatment of this topic, as well as many bibliographic references, we refer to the books of Ciarlet [12, 13]. To the ...
Motion of a charged particle in an EM field
... and v1 are small perturbations due to inhomogeneity. Next we split B into two parts B = B0 + B1 Where B0 = (0, 0, B0z ) is the main part, and B1 is a small disturbance - the source of our inhomogeneity. The equation of motion becomes mv̇ = q(v × B) = q((v0 + v1 ) × (B0 + B1 )) = q(v0 × B0 ) + q(v0 × ...
... and v1 are small perturbations due to inhomogeneity. Next we split B into two parts B = B0 + B1 Where B0 = (0, 0, B0z ) is the main part, and B1 is a small disturbance - the source of our inhomogeneity. The equation of motion becomes mv̇ = q(v × B) = q((v0 + v1 ) × (B0 + B1 )) = q(v0 × B0 ) + q(v0 × ...
