the capture of magnetic inelastic dark matter in the sun.
... Super-Kamiokande and IceCube. We find that we can put very strong bounds on this type of Dark Matter in a somewhat model independent way. Chapter 2 of this work presents a brief review of the evidence for Dark Matter, what we know of its properties and how it can be detected before introducing the m ...
... Super-Kamiokande and IceCube. We find that we can put very strong bounds on this type of Dark Matter in a somewhat model independent way. Chapter 2 of this work presents a brief review of the evidence for Dark Matter, what we know of its properties and how it can be detected before introducing the m ...
Defining and detecting quantum speedup
... consensus may be time- and community-dependent [14]. In the absence of a consensus about what is the best classical algorithm, we define potential (quantum) speedup as a speedup compared to a specific classical algorithm or a set of classical algorithms. An example is the simulation of the time evol ...
... consensus may be time- and community-dependent [14]. In the absence of a consensus about what is the best classical algorithm, we define potential (quantum) speedup as a speedup compared to a specific classical algorithm or a set of classical algorithms. An example is the simulation of the time evol ...
Optimal Detection of Symmetric Mixed Quantum States
... unitary group is not constrained to be Abelian. We obtain a convenient characterization of the LSM and show that the LSM operators have the same symmetries as the original state set. We then show that for such GU state sets, the probability of correctly detecting each of the states using the LSM is ...
... unitary group is not constrained to be Abelian. We obtain a convenient characterization of the LSM and show that the LSM operators have the same symmetries as the original state set. We then show that for such GU state sets, the probability of correctly detecting each of the states using the LSM is ...
Free particles from Brauer algebras in complex matrix models David Turton
... Brauer basis of operators The Brauer algebra can be used to build an orthogonal basis, as follows: The representations of the Brauer algebra are labelled by γ = (k, γ+ , γ− ) where k is an integer in the range 0 ≤ k ≤ min(m, n) (γ+ , γ− ) have m − k and n − k boxes respectively and form a form a co ...
... Brauer basis of operators The Brauer algebra can be used to build an orthogonal basis, as follows: The representations of the Brauer algebra are labelled by γ = (k, γ+ , γ− ) where k is an integer in the range 0 ≤ k ≤ min(m, n) (γ+ , γ− ) have m − k and n − k boxes respectively and form a form a co ...
electromagnetic energy-momentum tensor within material media
... RICHARDS into account, we find that ABRAHAM ' S and MINKOwsKI ' s tensors ar e equivalent in the following sense : ABRAHAM'S force density excites the constituent dipoles of the material and produces a mechanical momentum whic h travels together with the field . If we count this mechanical momentu m ...
... RICHARDS into account, we find that ABRAHAM ' S and MINKOwsKI ' s tensors ar e equivalent in the following sense : ABRAHAM'S force density excites the constituent dipoles of the material and produces a mechanical momentum whic h travels together with the field . If we count this mechanical momentu m ...
Physics at the FQMT`04 conference
... then called a closed system. The dynamics of a closed system are governed by the unitary evolution which is described either by the Schrödinger equation for the wave function or the Liouville equation for the density matrix of the system. Very often the needed (relevant) observables are single part ...
... then called a closed system. The dynamics of a closed system are governed by the unitary evolution which is described either by the Schrödinger equation for the wave function or the Liouville equation for the density matrix of the system. Very often the needed (relevant) observables are single part ...
Physics (PHYS)
... Observational Astrophysics This course provides an overview of astrophysics and introduces the student to the many conventions, units, coordinate systems, and nomenclature used in astrophysics. The course will survey observational, stellar, and extragalactic astrophysics as well as cosmology. The co ...
... Observational Astrophysics This course provides an overview of astrophysics and introduces the student to the many conventions, units, coordinate systems, and nomenclature used in astrophysics. The course will survey observational, stellar, and extragalactic astrophysics as well as cosmology. The co ...
Quantum Computation and Quantum Information 10th Anniversary
... In praise of the book 10 years after publication Ten years after its initial publication, “Mike and Ike” (as it’s affectionately called) remains the quantum computing textbook to which all others are compared. No other book in the field matches its scope: from experimental implementation to complexi ...
... In praise of the book 10 years after publication Ten years after its initial publication, “Mike and Ike” (as it’s affectionately called) remains the quantum computing textbook to which all others are compared. No other book in the field matches its scope: from experimental implementation to complexi ...
Dynamical Systems Method for Solving Operator Equations
... where B(u0 , R) = {u : ||u − u0 || ≤ R}, F ′ (u) is the Fréchet derivative (F-derivative) of the operator-function F at the point u, and the constant m(R) > 0 may grow arbitrarily as R grows. If (4) fails, we call problem (1) ill-posed. If problem (1) is ill-posed, we write it often as F (u) = f an ...
... where B(u0 , R) = {u : ||u − u0 || ≤ R}, F ′ (u) is the Fréchet derivative (F-derivative) of the operator-function F at the point u, and the constant m(R) > 0 may grow arbitrarily as R grows. If (4) fails, we call problem (1) ill-posed. If problem (1) is ill-posed, we write it often as F (u) = f an ...
simple harmonic motion
... The mass starts from rest (v = 0) some distance x from equilibrium. A force acting on the mass towards the centre (and therefore acceleration a too) is a maximum. The mass moves towards the centre gaining speed until it is moving fastest through the equilibrium point. The direction of the force chan ...
... The mass starts from rest (v = 0) some distance x from equilibrium. A force acting on the mass towards the centre (and therefore acceleration a too) is a maximum. The mass moves towards the centre gaining speed until it is moving fastest through the equilibrium point. The direction of the force chan ...
Damped Harmonic Oscillator with Applied Force
... A glass prism and rain can break light into its component colors. This is due to the index of refraction changing slightly with frequency. Why is that? Light is bent on going from one medium to another due to the differences in the speed of light between the mediums. We use the index of refraction t ...
... A glass prism and rain can break light into its component colors. This is due to the index of refraction changing slightly with frequency. Why is that? Light is bent on going from one medium to another due to the differences in the speed of light between the mediums. We use the index of refraction t ...
Efimov Trimers under Strong Confinement
... scaling symmetry, where the low-energy properties simply scale with a. It is then natural to ask how these Efimov trimers evolve once the bosons are subject to confinement and the motion is constrained. Cold-atom experiments already require the presence of a weak trapping potential, but the remarkab ...
... scaling symmetry, where the low-energy properties simply scale with a. It is then natural to ask how these Efimov trimers evolve once the bosons are subject to confinement and the motion is constrained. Cold-atom experiments already require the presence of a weak trapping potential, but the remarkab ...
