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Angular momentum circular states

Since the spin operator commutes with the momentum operator, it is possible to speak of states of definite momentum p and spin component /x. The components of the polarization vector may be chosen in such a way that e = XP- The two possible polarizations correspond to only two values of the component of spin angular momentum y,. The third value is excluded by the condition of tranversality. If the z-axis is directed along p, then x0 s excluded. The two vectors Xi and X2> corresponding to circular polarization are equivalent, respectively to Xi and X-i- Thus, the value17 of the spin component y = 1 corresponds to right circular polarization, while /z = — 1 corresponds to left circular polarization. [Pg.256]

In his 1913 papers Bohr developed a theory of the stationary states of the hydrogen atom. According to his theory the electron was to be considered as moving in a circular orbit about the proton. The amount of angular momentum for a stationary tate was assumed by Bohr to be equal to nh/2w, with n = 1, 2, 3, . J n Appendix II there is given the derivation of the energy values fcr the Bohr circular orbits. For... [Pg.33]

Fio. 2-3.—At the left is represented the circular orbit of the Bohr atom. At the right is shown the very eccentric orbit (line orbit), with no angular momentum, that corresponds somewhat more closely to the description of the hydrogen atom in its normal state given by quantum mechanics. [Pg.35]

In any low angular momentum state the radiative decay rate is usually dominated by the high frequency transitions to low lying states, and as a result it is impossible to control completely the decay rate using a millimeter wave cavity. In a circular i = m = n - 1 state the only decay is the far infrared transition to the n — 1 level, and Hulet et al. have observed the suppression of the decay of this level.26 They produced a beam of Cs atoms in the circular n = 22, = m = 21 state by pulsed laser excitation and an adiabatic rapid passage technique.27 The beam of circular state atoms then passed between a pair of plates 6.4 cm wide, 12.7 cm long, spaced by 230.1 jum, and held at 6 K. The 0 K radiative lifetime is 460ps, and... [Pg.63]

The action of a circularly polarised pulse leads to a repopulation of electrons and holes between states with a different angular momentum component in the direction of the pump pulse wave vector. The corresponding SIFE relaxation time describes the recovery of the symmetry of the initial angular momentum distribution. Again it is preferable that the probe response is dominated by intraband transitions or else inelastic scattering may obscure the relaxation of hot electron (hole) angular momentum. [Pg.218]

Fig. 2.2. Isometric projections of probability density pb(0, Fig. 2.2. Isometric projections of probability density pb(0,<p) of angular momentum distribution in an excited molecular state (a) denotes a Q-transition (linear polarized excitation) (b) denotes P- or -transition (linear polarized excitation) (c) denotes U-transition (excitation by righthanded circular polarized light).
Structure Whereas the remaining e stays in the Is ground orbital, the captured p occupies a large-(n, l) state n no = JM /rne 38, where M is the reduced mass of the p-He system. The angular momentum l which is brought by the captured p can be as much as that of the circular state, l n — 1. As shown in Fig. 1, the p is orbiting in a classical trajectory, while the e is distributed quantum mechanically. [Pg.247]

The energies of macroscopic objects, as well as those of microscopic objects, are quantized, but the effects of the quantization are not seen because the difference in energy between adjacent states is so small. Apply Bohr s quantization of angular momentum to the revolution of Earth (mass 6.0 X 10 " kg), which moves with a velocity of 3.0 X 10" m s in a circular orbit (radius 1.5 X 10 m) about the sun. The sun can be treated as fixed. Calculate the value of the quantum number n for the present state of the Earth-sun system. What would be the effect of an increase in by 1 ... [Pg.167]

Problem 6-1. Consider an electron moving in a circular orbit about a nucleus of charge Ze. Show that when the centrifugal force is just balanced by the centripetal force Ze2/ -8, the total energy is equal to one-half the potential energy —Ze2/r. Evaluate the energy of the stationary states for which the angular momentum equals nh/2ir, with n = 1, 2, 3, . ... [Pg.28]

The method works particularly well for ATI spectra excited by circularly polarised light. The reason for this is as follows an atom which absorbs N photons then acquires Nh units of angular momentum. The emerging electron is then subject to a repulsive centrifugal barrier (see chapter 5) and does not therefore penetrate into the core. Consequently, most atomic effects are suppressed, and a final state representation as a Volkov wavefunction is a reasonable approximation. This is also why intensity suppression occurs near threshold in this case the effect is very similar to delayed onset in single-photon ionisation to continua of high angular momentum. [Pg.350]

Fig. 9.7. Comparison between experimental data and KFR calculations, which demonstrates that the main features of ATI for circularly polarised light (including angular momentum barrier effects) are well accounted for in a non-perturbative model using Volkov final states (after H. Reiss [496]). Fig. 9.7. Comparison between experimental data and KFR calculations, which demonstrates that the main features of ATI for circularly polarised light (including angular momentum barrier effects) are well accounted for in a non-perturbative model using Volkov final states (after H. Reiss [496]).
Now consider what happens when a atom is at a position in space where the polarization is circular a" ", that is, with positive angular momentum of the li t along the axis of quantization. An atom at that place will be optically pumped into the state of highest projection of the atomic angular momentum along the quanti2 ition axis, m = +1/2. This is also the state that has the... [Pg.22]

Stationary states exist in which the energy of the electron is constant such states are characterized by circular orbits about the nucleus in which the electron has an angular momentum mvr given by equation 1.6. The integer, n, is the principal quantum number. [Pg.5]


See other pages where Angular momentum circular states is mentioned: [Pg.217]    [Pg.217]    [Pg.54]    [Pg.259]    [Pg.34]    [Pg.574]    [Pg.633]    [Pg.35]    [Pg.367]    [Pg.3]    [Pg.11]    [Pg.286]    [Pg.2]    [Pg.6]    [Pg.192]    [Pg.275]    [Pg.248]    [Pg.190]    [Pg.13]    [Pg.6068]    [Pg.6069]    [Pg.29]    [Pg.49]    [Pg.248]    [Pg.144]    [Pg.112]    [Pg.204]    [Pg.205]    [Pg.155]    [Pg.462]    [Pg.327]    [Pg.121]    [Pg.123]    [Pg.28]    [Pg.382]    [Pg.3]    [Pg.155]   
See also in sourсe #XX -- [ Pg.26 , Pg.27 , Pg.28 , Pg.29 , Pg.30 ]




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Angular momentum

Circular states

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