950 - IACR
... be useful only for a limited time: currently, we may assume a small limit on the adversary’s quantum memory. Should quantum technology advance, though, quantum memory might become cheap, and at that point BQSM protocols must not be used any more. In contrast, with everlasting security as in this pap ...
... be useful only for a limited time: currently, we may assume a small limit on the adversary’s quantum memory. Should quantum technology advance, though, quantum memory might become cheap, and at that point BQSM protocols must not be used any more. In contrast, with everlasting security as in this pap ...
Toward the Unification of Physics and Number Theory
... Fundamental particles have distinct geometries and are, in some sense, geometric symbols. For example, at each energy state, an orbiting electron forms a finite set of shape-symbols – p-orbital geometries composed of the probability distribution of the wave-function in 3space. There are strict rules ...
... Fundamental particles have distinct geometries and are, in some sense, geometric symbols. For example, at each energy state, an orbiting electron forms a finite set of shape-symbols – p-orbital geometries composed of the probability distribution of the wave-function in 3space. There are strict rules ...
On a measurement-free quantum lambda calculus with classical
... classical case. In addition to the concrete technical problems (up to now it has been difficult to build even very simple quantum circuits), there is the necessity of developing adequate calculi of quantum computable functions. In particular, it is not clear how the idea of having functions as ‘first-c ...
... classical case. In addition to the concrete technical problems (up to now it has been difficult to build even very simple quantum circuits), there is the necessity of developing adequate calculi of quantum computable functions. In particular, it is not clear how the idea of having functions as ‘first-c ...
Asymptotic Safety in Quantum Gravity and Diffeomorphic Non
... ρ(r = 0+ ; M ) = 2GM , ρ(r = 0) = 0, can effectively be interpreted as saying that the “point” mass has a finite area but zero volume [11]. It is generally believed that any quantum theory of gravity should have a generic feature, a quantum of length, which can be taken to coincide with the Planck s ...
... ρ(r = 0+ ; M ) = 2GM , ρ(r = 0) = 0, can effectively be interpreted as saying that the “point” mass has a finite area but zero volume [11]. It is generally believed that any quantum theory of gravity should have a generic feature, a quantum of length, which can be taken to coincide with the Planck s ...
Lab 3: Electric Fields II
... Gravity, you remember, is not a force that acts when two objects touch. It is a force that seems to act over a distance. Physicists have never been happy with the idea of “action-at-a-distance.” Rather, they prefer to think about a gravitational field that is created by one object, like the sun. The ...
... Gravity, you remember, is not a force that acts when two objects touch. It is a force that seems to act over a distance. Physicists have never been happy with the idea of “action-at-a-distance.” Rather, they prefer to think about a gravitational field that is created by one object, like the sun. The ...
Experimental nonlocal and surreal Bohmian trajectories
... (WWM) device, the particle’s Bohmian trajectories can display seemingly contradictory behavior: There are instances when the particle’s Bohmian trajectory goes through one slit, and yet the WWM result indicates that it had gone through the other slit. ESSW concluded that these trajectories predicted ...
... (WWM) device, the particle’s Bohmian trajectories can display seemingly contradictory behavior: There are instances when the particle’s Bohmian trajectory goes through one slit, and yet the WWM result indicates that it had gone through the other slit. ESSW concluded that these trajectories predicted ...
What is the Entropy in Entropic Gravity?
... The existence of a profound relationship between gravity and entropy has been recognized since the formulation of the laws of black hole mechanics [1] and the derivation of the BekensteinHawking entropy [2, 3]. More recently, ideas such as the holographic principle [4, 5], black hole complementarity ...
... The existence of a profound relationship between gravity and entropy has been recognized since the formulation of the laws of black hole mechanics [1] and the derivation of the BekensteinHawking entropy [2, 3]. More recently, ideas such as the holographic principle [4, 5], black hole complementarity ...
RLE_PR_140_02_01s
... the existence, action, period, and stability of the closed orbits of the classical system. However, there is much more to know about the classical motione.g., initial conditions and trajectories. Previously, all studies of recurrence spectra have used static fields. We have taken a new approach by i ...
... the existence, action, period, and stability of the closed orbits of the classical system. However, there is much more to know about the classical motione.g., initial conditions and trajectories. Previously, all studies of recurrence spectra have used static fields. We have taken a new approach by i ...
Studies of Highly Polar Atomic and Molecular Systems: Quantum Dynamics Investigations
... The goal of the Trent Optical Physics Laboratory is the investigation of quantum dynamics and the production and manipulation of heavy Rydberg systems composed of lithium ions. This requires devising the theoretical framework for understanding two-level quantum dynamics, covered in Chapter 3 and app ...
... The goal of the Trent Optical Physics Laboratory is the investigation of quantum dynamics and the production and manipulation of heavy Rydberg systems composed of lithium ions. This requires devising the theoretical framework for understanding two-level quantum dynamics, covered in Chapter 3 and app ...
Section D: - Curved Force Line Elements Theory
... had begun with Yang and Mills in 1954, who introduced the equivalent of an isospin for P and N. They defined a weak isospin Tw for a lepton, with ν having a Twz = + and e– having a Twz = − . This weak isospin has nothing to do with the usual isospin, but from the standpoint of a Yang–Mills type of g ...
... had begun with Yang and Mills in 1954, who introduced the equivalent of an isospin for P and N. They defined a weak isospin Tw for a lepton, with ν having a Twz = + and e– having a Twz = − . This weak isospin has nothing to do with the usual isospin, but from the standpoint of a Yang–Mills type of g ...
Exploring a Classical Model of the Helium Atom
... understanding of energy levels and orbits and to the difficulty of calculating trajectories. Those who made these studies adopted only trivial periodic orbits, satisfying trivial symmetry, which turned out to be unstable. As for the correct understanding of quantum-classical correspondence, we had t ...
... understanding of energy levels and orbits and to the difficulty of calculating trajectories. Those who made these studies adopted only trivial periodic orbits, satisfying trivial symmetry, which turned out to be unstable. As for the correct understanding of quantum-classical correspondence, we had t ...
Quantum defect theory description of weakly bound levels and Feshbach...
... In some applications, MQDT is employed in an essentially exact manner, in that accurate solutions of the close-coupling equations are obtained out to a distance around r0 = 30–50 a.u., and then matched to linear combinations of single channel solutions (fi , gi ) in the appropriate long range potent ...
... In some applications, MQDT is employed in an essentially exact manner, in that accurate solutions of the close-coupling equations are obtained out to a distance around r0 = 30–50 a.u., and then matched to linear combinations of single channel solutions (fi , gi ) in the appropriate long range potent ...
PowerPoint Presentation - Lecture 1 Electric Charge*
... “touch it”? Even in a vacuum! We say there is a field produced by q1 that extends out in space everywhere. ...
... “touch it”? Even in a vacuum! We say there is a field produced by q1 that extends out in space everywhere. ...
