Quantum information processing with superconducting qubits in a
... Cooper-pair box and a cavity photon mode undergoes Rabi oscillations and propose a new quantum computing scheme based on Josephson charge qubits [19]. The microwave-controlled approach proposed in our paper has the significant advantage that any two qubits (not necessarily neighbors) can be effectiv ...
... Cooper-pair box and a cavity photon mode undergoes Rabi oscillations and propose a new quantum computing scheme based on Josephson charge qubits [19]. The microwave-controlled approach proposed in our paper has the significant advantage that any two qubits (not necessarily neighbors) can be effectiv ...
Slide 1
... • Vortex core size on the optical lattice is about 2 microns. Focus the probe laser beam to this size and scan the lattice to determine the particle density distribution. ...
... • Vortex core size on the optical lattice is about 2 microns. Focus the probe laser beam to this size and scan the lattice to determine the particle density distribution. ...
Chapter 21
... The interaction between charges was analyzed as a charge exerting a force on another charge (Coulomb’s Law). Another way to analyze the interaction is to say that one charge is interacting with the “electric field” produced by the other charge. That is, a charge placed at a particular position in sp ...
... The interaction between charges was analyzed as a charge exerting a force on another charge (Coulomb’s Law). Another way to analyze the interaction is to say that one charge is interacting with the “electric field” produced by the other charge. That is, a charge placed at a particular position in sp ...
Relativistic Quantum Mechanics
... precess with the Larmor frequency and the angle of the precession is easily calculated as a function of the strength of the magnetic field. After passing through the magnetic field, the beam interfers with the second beam which followed a path outside the magnetic field. As demonstrated ...
... precess with the Larmor frequency and the angle of the precession is easily calculated as a function of the strength of the magnetic field. After passing through the magnetic field, the beam interfers with the second beam which followed a path outside the magnetic field. As demonstrated ...
Classical analogy of Fano resonances
... before it meets the zero-frequency ωzero , the first oscillator settles into steady-state motion (i.e., the transient motion has already decayed) and the displacement x1 is eventually π out of phase with respect to the external force. Next, as the frequency passes through the anti-resonance at ω = ω ...
... before it meets the zero-frequency ωzero , the first oscillator settles into steady-state motion (i.e., the transient motion has already decayed) and the displacement x1 is eventually π out of phase with respect to the external force. Next, as the frequency passes through the anti-resonance at ω = ω ...
Nuclear Fusion and Radiation
... If Ek (0) is too large, the particle will escape. Note that although E⊥ (0)/ET (0) may satisfy the reflection condition at injection, coulomb scattering collisions will alter the orientation of the particle with respect to E . Thus, we must average the assembly of particles over all orientations to ...
... If Ek (0) is too large, the particle will escape. Note that although E⊥ (0)/ET (0) may satisfy the reflection condition at injection, coulomb scattering collisions will alter the orientation of the particle with respect to E . Thus, we must average the assembly of particles over all orientations to ...
E - ckw
... The conductor itself carries a net charge of 1 C, and there’s a 2 C point charge inside the cavity. Find the net charge on the cavity wall & on the outer surface of the conductor, assuming electrostatic equilibrium. ...
... The conductor itself carries a net charge of 1 C, and there’s a 2 C point charge inside the cavity. Find the net charge on the cavity wall & on the outer surface of the conductor, assuming electrostatic equilibrium. ...
Were Bohr and Einstein both right
... in terms of a energy function / Hamiltonian as in quantum theory, and in the urs arising from the fact that (E2 – p2 – m2) = 0 where E is the energy, p the momentum, m the mass; a relativistic equation which leads to Einstein's famous E = mc2 . • for any measurement, there must exist a measurement s ...
... in terms of a energy function / Hamiltonian as in quantum theory, and in the urs arising from the fact that (E2 – p2 – m2) = 0 where E is the energy, p the momentum, m the mass; a relativistic equation which leads to Einstein's famous E = mc2 . • for any measurement, there must exist a measurement s ...
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... This physical quantum gravity state has a good classical limit (i.e.,. a DeSitter spacetime for small cosmological constant, hence large k). So when Smolin talks of spinet-based physical states, their classical limit are the beable geometries. How do we interpret this in terms of Bohm's pilot-wave ...
... This physical quantum gravity state has a good classical limit (i.e.,. a DeSitter spacetime for small cosmological constant, hence large k). So when Smolin talks of spinet-based physical states, their classical limit are the beable geometries. How do we interpret this in terms of Bohm's pilot-wave ...
