Intermolecular interactions
... = Etot (R) − EA − EB The intermolecular pair-potential is the work to bring together the two systems from infinity to the distance R, against the intermolecular force, F (R) Z ∞ U (R) = ...
... = Etot (R) − EA − EB The intermolecular pair-potential is the work to bring together the two systems from infinity to the distance R, against the intermolecular force, F (R) Z ∞ U (R) = ...
Voltage-dependent electron distribution in a small spin valve
... gradual evolution of the magnetization, activated behavior at low temperatures, and precession states with small precession angles.7 Such precession states present a problem for theory,1 since the Landau-Lifshitz equation, which is at the basis of Ref. 1 implies large precession angles.5,25,26 The a ...
... gradual evolution of the magnetization, activated behavior at low temperatures, and precession states with small precession angles.7 Such precession states present a problem for theory,1 since the Landau-Lifshitz equation, which is at the basis of Ref. 1 implies large precession angles.5,25,26 The a ...
On convected wave structures and spectral transfer in space
... in the ecliptic (Parker, 1958). Close to the corona, its direction is rather radial, while the angle between outflow direction and interplanetary magnetic field increases with distance from Sun. The first ideas about a more or less steady corpuscular outflow from the Sun were confirmed based on obse ...
... in the ecliptic (Parker, 1958). Close to the corona, its direction is rather radial, while the angle between outflow direction and interplanetary magnetic field increases with distance from Sun. The first ideas about a more or less steady corpuscular outflow from the Sun were confirmed based on obse ...
Estudio desde primeros principios de mecanismos de apantallado
... ferromagnets, as they both exhibit a hysteresis loop when polarization (magnetization ...
... ferromagnets, as they both exhibit a hysteresis loop when polarization (magnetization ...
Modeling motion - Union College Blogging
... We will now introduce how to model motion with a computer. You will write program that will model the motion of a “fan cart” on a track, which experiences a constant force of interaction due to the action of the small electric fan mounted onto the cart. ...
... We will now introduce how to model motion with a computer. You will write program that will model the motion of a “fan cart” on a track, which experiences a constant force of interaction due to the action of the small electric fan mounted onto the cart. ...
Timing of the accreting millisecond pulsar IGR J17511-3057
... to model residuals in the iron range, though this feature is probably due to the contamination of the Galactic ridge in the field of view of the PCA (Markwardt et al. 2009b). The reduced chisquare of the fit is good (χ2r = 64.3/72). The unabsorbed flux we detect in the 3–50 keV band is 1.14(1) × 10− ...
... to model residuals in the iron range, though this feature is probably due to the contamination of the Galactic ridge in the field of view of the PCA (Markwardt et al. 2009b). The reduced chisquare of the fit is good (χ2r = 64.3/72). The unabsorbed flux we detect in the 3–50 keV band is 1.14(1) × 10− ...