March 2002 Vol - Basarab Nicolescu
... to the quantum laws, which are on radical break with the laws of the macrophysical world. This means that two levels of Reality are different if, passing from one to another, there is a break of the laws and break of the fundamental concepts (as causality, for example). The discontinuity present in ...
... to the quantum laws, which are on radical break with the laws of the macrophysical world. This means that two levels of Reality are different if, passing from one to another, there is a break of the laws and break of the fundamental concepts (as causality, for example). The discontinuity present in ...
Heavy Ion Physics from RHIC to LHC Joe Kapusta
... Numerical Hydrodynamics Model parameters fixed by and p at b 0, the rest are prediction s (Heinz and Kolb) H RHIC / H Universe 2 10 40 ...
... Numerical Hydrodynamics Model parameters fixed by and p at b 0, the rest are prediction s (Heinz and Kolb) H RHIC / H Universe 2 10 40 ...
Moving Lonely Electrons WAVES
... wave function as in Figure 11-1(a). The electron can have many different momenta. (Remember we needed all those momenta to construct its wave function.) Of course, it also has a range of possible locations. So, we don’t quite know where it is, and we don’t quite know how fast it is moving — an uncer ...
... wave function as in Figure 11-1(a). The electron can have many different momenta. (Remember we needed all those momenta to construct its wave function.) Of course, it also has a range of possible locations. So, we don’t quite know where it is, and we don’t quite know how fast it is moving — an uncer ...
Validity of Semiclassical Gravity in the Stochastic Gravity Approach
... equation. Following these approaches the Minkowski metric is shown to be a stable solution of semiclassical gravity with respect to small metric perturbations. As emphasized in Ref. [23] the above criteria may be understood as criteria within semiclassical gravity itself. It is certainly true that s ...
... equation. Following these approaches the Minkowski metric is shown to be a stable solution of semiclassical gravity with respect to small metric perturbations. As emphasized in Ref. [23] the above criteria may be understood as criteria within semiclassical gravity itself. It is certainly true that s ...
Document
... General security proofs of QKD system: 1. Alice and Bob apply random permutations to their systems. 2. De Finetti argument follows. 3. After sequences of state preparations and measurements, they obtain information about their connecting quantum channel, or equivalently, about the virtual bipartite ...
... General security proofs of QKD system: 1. Alice and Bob apply random permutations to their systems. 2. De Finetti argument follows. 3. After sequences of state preparations and measurements, they obtain information about their connecting quantum channel, or equivalently, about the virtual bipartite ...
Phys. Rev. Lett. 103, 025301 (2009).
... Graphene [1,2], attracts a lot of attention due to the massless relativistic dispersion of its quasiparticles and their high mobility. Recently, it was shown that this material offers a unique opportunity to observe transport properties of a plasma of ultrarelativistic particles at moderately high t ...
... Graphene [1,2], attracts a lot of attention due to the massless relativistic dispersion of its quasiparticles and their high mobility. Recently, it was shown that this material offers a unique opportunity to observe transport properties of a plasma of ultrarelativistic particles at moderately high t ...
Document
... • FCQs will take place on Wednesday at the beginning of class. • The last homework set will be out on 4/22 and will be due on Thursday 4/30 (one day later than normal). ...
... • FCQs will take place on Wednesday at the beginning of class. • The last homework set will be out on 4/22 and will be due on Thursday 4/30 (one day later than normal). ...
Time-dependent quantum circular billiard
... by Makowski et al. [16]. We solve the Schr¨odinger equation for the circular billiard with a time-dependent radius. In particular, we consider the following cases: i) monotonically expanding (contracting) circle; ii) non-harmonically breathing circle; iii) harmonically breathing circle. The classica ...
... by Makowski et al. [16]. We solve the Schr¨odinger equation for the circular billiard with a time-dependent radius. In particular, we consider the following cases: i) monotonically expanding (contracting) circle; ii) non-harmonically breathing circle; iii) harmonically breathing circle. The classica ...
ENTANGLEMENT I by Robert Nemiroff Physics X
... ENTANGLEMENT: LOCALITY The principle of locality states that objects can only be affected by their immediate surroundings. Entanglement appears to violate locality but not in such a way that allows distant observers to send information to each other faster than the speed of light. ...
... ENTANGLEMENT: LOCALITY The principle of locality states that objects can only be affected by their immediate surroundings. Entanglement appears to violate locality but not in such a way that allows distant observers to send information to each other faster than the speed of light. ...
A true Science Adventure - Wave Structure of Matter (WSM)
... probability interpretation of his own Schrödinger’s Equation, he firmly disagreed with Bohr and mainstream quantum mechanics and wrote3: Let me say at the outset, that in this discourse, I am opposing not a few special statements of quantum mechanics held today (1950s), I am opposing as it were the ...
... probability interpretation of his own Schrödinger’s Equation, he firmly disagreed with Bohr and mainstream quantum mechanics and wrote3: Let me say at the outset, that in this discourse, I am opposing not a few special statements of quantum mechanics held today (1950s), I am opposing as it were the ...
Black Stars, Not Holes
... essentially no light or other radiation of their own. Although these dark objects have masses ranging from just a few suns to well over a million suns, their diameters, as best astrophysicists can determine, range from only several kilometers to millions of kilometers— matching general relativity’s ...
... essentially no light or other radiation of their own. Although these dark objects have masses ranging from just a few suns to well over a million suns, their diameters, as best astrophysicists can determine, range from only several kilometers to millions of kilometers— matching general relativity’s ...
General Mathematical Description of a Quantum System
... Normalized states are states which have a direct probability interpretation. It is mathematically convenient to permit the use of states whose norms are not equal to unity, but it is necessary in order to make use of the probability interpretation to deal only with the normalized state which has nor ...
... Normalized states are states which have a direct probability interpretation. It is mathematically convenient to permit the use of states whose norms are not equal to unity, but it is necessary in order to make use of the probability interpretation to deal only with the normalized state which has nor ...
Two-particle Harmonic Oscillator in a One
... where c = {c1 , c2 , . . . , cN } are linear variational parameters, which would give rise to the well known RayleighRitz secular equations, and a is a nonlinear variational parameter. Even the simplest and crudest variational functions provide reasonable results for all values of λ, as shown in Sec ...
... where c = {c1 , c2 , . . . , cN } are linear variational parameters, which would give rise to the well known RayleighRitz secular equations, and a is a nonlinear variational parameter. Even the simplest and crudest variational functions provide reasonable results for all values of λ, as shown in Sec ...
Classical and Non-Classical Representations in Physics
... possible states is called the state space. The evolution of the system can then be described by a timeparametrized trajectory in the state space, representing the states of the system at subsequent instants. In order to determine the trajectory, one needs two further structures: operators and dynami ...
... possible states is called the state space. The evolution of the system can then be described by a timeparametrized trajectory in the state space, representing the states of the system at subsequent instants. In order to determine the trajectory, one needs two further structures: operators and dynami ...