Resolving Spin-Orbit- and Hyperfine
... behavior in the frequency or field sweep direction. The behavior of the EDSR peaks as a function of MW power is shown in Fig. 2(b). For very low MW powers, the width of the EDSR signal is very sensitive to the MW power while for high MW powers the linewidth saturates [Fig. 2(b) inset]. Furthermore, ...
... behavior in the frequency or field sweep direction. The behavior of the EDSR peaks as a function of MW power is shown in Fig. 2(b). For very low MW powers, the width of the EDSR signal is very sensitive to the MW power while for high MW powers the linewidth saturates [Fig. 2(b) inset]. Furthermore, ...
Many-body theory
... large number of particles. The reason is the equivalence of particles, a genuine quantum effect, which requires the (anti)symmetrization of the wave functions. The resulting wave functions are too complicated for any useful calculation. Another representation of the many particle system, based on th ...
... large number of particles. The reason is the equivalence of particles, a genuine quantum effect, which requires the (anti)symmetrization of the wave functions. The resulting wave functions are too complicated for any useful calculation. Another representation of the many particle system, based on th ...
Chapter 2: Atomic Structure and Inter-atomic Bonding
... Electron Spin Quantum Number, s The third of these quantum numbers is called the electron spin quantum number, s, which designates the spin moment. There are only two values: +½ and -½. These are also referred to as 'spin up' and 'spin down'. This number is used to explain behavior of individual ele ...
... Electron Spin Quantum Number, s The third of these quantum numbers is called the electron spin quantum number, s, which designates the spin moment. There are only two values: +½ and -½. These are also referred to as 'spin up' and 'spin down'. This number is used to explain behavior of individual ele ...
detail links - Shanghai Institute of Technical Physics
... nm. GaAs QDs are considered here. The effective masses of electrons and holes are m e = 0.067 and mh = 0.51, respectively, in the unit of electron rest mass, and the band gap is E g = 1.51914 eV [26]. The corresponding ground-state exciton resonance frequency ω 0 of QDs is then given as 1.535 eV [5] ...
... nm. GaAs QDs are considered here. The effective masses of electrons and holes are m e = 0.067 and mh = 0.51, respectively, in the unit of electron rest mass, and the band gap is E g = 1.51914 eV [26]. The corresponding ground-state exciton resonance frequency ω 0 of QDs is then given as 1.535 eV [5] ...
Lokal fulltext - Chalmers tekniska högskola
... mediated by force-bearing particles known as bosons: the graviton, the photon, the W and Z-bosons of the weak interaction and the gluons which mediate the strong interaction. And finally, the now most well-known of them all, the Higgs boson, representing the interaction with the Higgs field through ...
... mediated by force-bearing particles known as bosons: the graviton, the photon, the W and Z-bosons of the weak interaction and the gluons which mediate the strong interaction. And finally, the now most well-known of them all, the Higgs boson, representing the interaction with the Higgs field through ...
Does a Relativistic Theory Always Have a Non
... and which can be regarded as different non-relativistic limits of standard Maxwell theory. It is the so-called “magnetic limit” (see below) which involves transformations of the potentials under boosts that appear in the Galilean covariant version of both classical and quantum mechanics. Both limits ...
... and which can be regarded as different non-relativistic limits of standard Maxwell theory. It is the so-called “magnetic limit” (see below) which involves transformations of the potentials under boosts that appear in the Galilean covariant version of both classical and quantum mechanics. Both limits ...
Spin and its applications - beim Quantum Spin
... You may complain about that. But just remember that you were happy enough to talk about the mass of an object without anyone ever telling you what it actually is. ...
... You may complain about that. But just remember that you were happy enough to talk about the mass of an object without anyone ever telling you what it actually is. ...
Dynamical generation of wormholes with charged fluids in quadratic Palatini gravity
... black hole solutions have been established [6]. In the context of modified gravity, Vaidya-type solutions have been found in metric fðRÞ gravity coupled to both Maxwell and non-Abelian Yang-Mills fields [7] and in Lovelock gravity [8]. The Vaidya metric has also been used to consider whether a wormh ...
... black hole solutions have been established [6]. In the context of modified gravity, Vaidya-type solutions have been found in metric fðRÞ gravity coupled to both Maxwell and non-Abelian Yang-Mills fields [7] and in Lovelock gravity [8]. The Vaidya metric has also been used to consider whether a wormh ...
The Proton Radius Puzzle
... electron, I should be able to show that pretty easily. Of course the mainstream can't possibly calculate this, since they simply give charged particles a ±1 charge. I have shown that is hopelessly naïve and how it causes many of their problems—not just this one. I have proved that in many previous p ...
... electron, I should be able to show that pretty easily. Of course the mainstream can't possibly calculate this, since they simply give charged particles a ±1 charge. I have shown that is hopelessly naïve and how it causes many of their problems—not just this one. I have proved that in many previous p ...
Correlated many-electron states in a quantum dot containing a
... Here i1 / iN↑ and j1 / jN↓ are the indices of single states for which each index is set by two quantum numbers 共radial and azimuthal quantum numbers兲, as mentioned above. The number of possible configurations NC depends on the number of electrons, Ne, the number of single orbitals, NS, and the size ...
... Here i1 / iN↑ and j1 / jN↓ are the indices of single states for which each index is set by two quantum numbers 共radial and azimuthal quantum numbers兲, as mentioned above. The number of possible configurations NC depends on the number of electrons, Ne, the number of single orbitals, NS, and the size ...
Is gravitational mass of a composite quantum body equivalent to its
... (e.g., a hydrogen atom) with an external gravitational field (e.g., the Earth). Our first result is that the equivalence between passive gravitational mass and energy may survive at a macroscopic level. In particular, we show that the quantum virial theorem [9] results in equality between the expect ...
... (e.g., a hydrogen atom) with an external gravitational field (e.g., the Earth). Our first result is that the equivalence between passive gravitational mass and energy may survive at a macroscopic level. In particular, we show that the quantum virial theorem [9] results in equality between the expect ...
1 The quantum-classical boundary and the moments of inertia of
... maximum temporal extent for any quantum wave. Since the time and frequency spectra of wave functions are related by a Fourier transform (Robinett), this limitation on the temporal extent of quantum waves then essentially causes every quantum wave in effect to become a wave packet, and accordingly le ...
... maximum temporal extent for any quantum wave. Since the time and frequency spectra of wave functions are related by a Fourier transform (Robinett), this limitation on the temporal extent of quantum waves then essentially causes every quantum wave in effect to become a wave packet, and accordingly le ...
Quantum Picture of the Josephson Junction
... are not equal. This is a significant quality of this system that makes it a candidate for qubit, as discussed later. The potential in my calculation and the eigenfunctions for the 4 lowest states are shown in Fig. 4. The eigenfunctions look similar with eigenfunctions of Harmonic Oscillator Potentia ...
... are not equal. This is a significant quality of this system that makes it a candidate for qubit, as discussed later. The potential in my calculation and the eigenfunctions for the 4 lowest states are shown in Fig. 4. The eigenfunctions look similar with eigenfunctions of Harmonic Oscillator Potentia ...
univERsity oF copEnhAGEn
... of spacetime is less than two, where one encounters the so-called non-critical string theory. This string theory can be solved both using standard continuum quantization and using the DT-lattice regularization (and taking the limit at → 0). Agreement is found. Thus a lattice regularization is not in ...
... of spacetime is less than two, where one encounters the so-called non-critical string theory. This string theory can be solved both using standard continuum quantization and using the DT-lattice regularization (and taking the limit at → 0). Agreement is found. Thus a lattice regularization is not in ...
Further Quantum Mechanics: Problem Set 2. Trinity term weeks 1 – 2
... In the β decay H3 (1 proton + 2 neutrons in the nucleus) → (He3 )+ (2 protons + 1 neutron in the nucleus), the emitted electron has a kinetic energy of 16 keV. We will consider the effects on the motion of the atomic electron, i.e. the one orbiting the nucleus, which we assume is initially in the gr ...
... In the β decay H3 (1 proton + 2 neutrons in the nucleus) → (He3 )+ (2 protons + 1 neutron in the nucleus), the emitted electron has a kinetic energy of 16 keV. We will consider the effects on the motion of the atomic electron, i.e. the one orbiting the nucleus, which we assume is initially in the gr ...
