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Binary rotation

OK, your molecule does not have a C5 axis. However, if it has a C4 axis, it also has three binary rotation axes collinear with the C4 and six other binary axes. Look carefully to be sure that your molecule indeed belongs to one of the octahedral groups. [Pg.191]

If there is neither a C5 axis nor a C4 axis, the symmetry of your molecule is that of one of the tetrahedral groups. Check that it also has four 3-fold and three binary rotation axes. [Pg.191]

Figure 4 The annihilation of neutrino-antineutrino pairs above the remnant of a neutron star merger drives relativistic jets along the original binary rotation axis (only upper half-plane is shown). The x-axis lies in the original binary orbital plane, the dark oval around the origin is the newly formed, probably unstable, supermassive neutron star formed in the coalescence. Color-coded is the asymptotic Lorentz-factor. Details can be found in Rosswog et al. 2003. Figure 4 The annihilation of neutrino-antineutrino pairs above the remnant of a neutron star merger drives relativistic jets along the original binary rotation axis (only upper half-plane is shown). The x-axis lies in the original binary orbital plane, the dark oval around the origin is the newly formed, probably unstable, supermassive neutron star formed in the coalescence. Color-coded is the asymptotic Lorentz-factor. Details can be found in Rosswog et al. 2003.
The above analysis shows that the set of turns To Tn E, E-, i = 1,2,3, provides a geometric realization of the quaternion group and thus establishes the connection between the quaternion units and turns through rc/2, and hence rotations through % (binary rotations). This suggests that the whole set of turns might provide a geometric realization of the set of unit quaternions. Section 12.5 will not only prove this to be the case, but will also provide us with the correct parameterization of a rotation. [Pg.227]

Example 12.6-1 The point group C2v = E C2z perpendicular axes, all operations except E are irregular and there is consequently only one doubly degenerate spinor representation, Ei/2. Contrast C 21, = E C2z / [ in which rrh is az = IC2z and thus an improper binary rotation about... [Pg.233]

Example 12.6-2 The classes of Td are E 4C3 3C2 6S4 6dihedral planes occur in three pairs of perpendicular improper BB rotations so both 3C2 and 6rrd are irregular classes. There are therefore Nv 5 vector representations and Ns = 3 spinor representations. [Pg.233]

Parameters that satisfy eq. (12) are referred to as standard quaternion (or Euler-Rodrigues) parameters. Note that A = sin(j(/>)n belongs to the positive hemisphere h for positive rotations and to —h for negative rotations. For binary rotations, n, and so X = 0, A = 1, and A belongs to h because there is no rotation R( n n). Therefore for any point group, h must be defined so as to contain the poles of all positive rotations, including binary rotations. Due to the range of , standard quaternion parameters must satisfy either... [Pg.235]

Example 12.6-3 Determine the PF for the multiplication of a binary rotation with itself. [Pg.235]

The stereograms include symbols to identify the locations of the symmetry elements of the structures with respect to the regular orbit points on the unit sphere. These are shown normally as filled polygons for proper rotational axes and empty polygons for improper rotations, which give rise to actions across the hemispherical plane, while binary rotations are shown as ellipses, either filled or empty, but mirror planes, the improper axes of binary rotation, are distinguished on the stereograms as solid lines. [Pg.57]

This character can be zero only for a = n and, hence, for binary rotations with n = 2. To examine whether or not the matrix for a binary rotation can be class-conjugated to minus itself, we may limit ourselves to the study of one orientation of the rotation axis, say C. Indeed, in SU 2) any orientation can always be transformed backward to this standard choice by a unitary transformation. The problem thus reduces to finding a spinor operation X represented by a matrix X with Cayley-Klein parameters ax,bx, which transforms (C ) into minus itself ... [Pg.179]

It is beyond the scope of these introductory notes to treat individual problems in fine detail, but it is interesting to close the discussion by considering certain, geometric phase related, symmetry effects associated with systems of identical particles. The following account summarizes results from Mead and Truhlar [10] for three such particles. We know, for example, that the fermion statistics for H atoms require that the vibrational-rotational states on the ground electronic energy surface of NH3 must be antisymmetric with respect to binary exchange... [Pg.28]

The catalytic subunit then catalyzes the direct transfer of the 7-phosphate of ATP (visible as small beads at the end of ATP) to its peptide substrate. Catalysis takes place in the cleft between the two domains. Mutual orientation and position of these two lobes can be classified as either closed or open, for a review of the structures and function see e.g. [36]. The presented structure shows a closed conformation. Both the apoenzyme and the binary complex of the porcine C-subunit with di-iodinated inhibitor peptide represent the crystal structure in an open conformation [37] resulting from an overall rotation of the small lobe relative to the large lobe. [Pg.190]

Storer model used in this theory enables us to describe classically the spectral collapse of the Q-branch for any strength of collisions. The theory generates the canonical relation between the width of the Raman spectrum and the rate of rotational relaxation measured by NMR or acoustic methods. At medium pressures the impact theory overlaps with the non-model perturbation theory which extends the relation to the region where the binary approximation is invalid. The employment of this relation has become a routine procedure which puts in order numerous experimental data from different methods. At low densities it permits us to estimate, roughly, the strength of collisions. [Pg.7]

The quantum theory of spectral collapse presented in Chapter 4 aims at even lower gas densities where the Stark or Zeeman multiplets of atomic spectra as well as the rotational structure of all the branches of absorption or Raman spectra are well resolved. The evolution of basic ideas of line broadening and interference (spectral exchange) is reviewed. Adiabatic and non-adiabatic spectral broadening are described in the frame of binary non-Markovian theory and compared with the impact approximation. The conditions for spectral collapse and subsequent narrowing of the spectra are analysed for the simplest examples, which model typical situations in atomic and molecular spectroscopy. Special attention is paid to collapse of the isotropic Raman spectrum. Quantum theory, based on first principles, attempts to predict the. /-dependence of the widths of the rotational component as well as the envelope of the unresolved and then collapsed spectrum (Fig. 0.4). [Pg.7]

Markovian perturbation theory as well as impact theory describe solely the exponential asymptotic behaviour of rotational relaxation. However, it makes no difference to this theory whether the interaction with a medium is a sequence of pair collisions or a weak collective perturbation. Being binary, the impact theory holds when collisions are well separated (tc < to) while the perturbation theory is broader. If it is valid, a new collision may start before the preceding one has been completed when To < Tc TJ = t0/(1 - y). [Pg.34]

The value of the magnetic hyperfine interaction constant C = 22.00 kHz is supposed to be reliably measured in the molecular beam method [71]. Experimental data for 15N2 are shown in Fig. 1.24, which depicts the density-dependence of T2 = (27tAv1/2)-1 at several temperatures. The fact that the dependences T2(p) are linear until 200 amagat proves that binary estimation of the rotational relaxation rate is valid within these limits and that Eq. (1.124) may be used to estimate cross-section oj from... [Pg.57]

As can be seen from the above, the shape of the resolved rotational structure is well described when the parameters of the fitting law were chosen from the best fit to experiment. The values of estimated from the rotational width of the collapsed Q-branch qZE. Therefore the models giving the same high-density limits. One may hope to discriminate between them only in the intermediate range of densities where the spectrum is unresolved but has not yet collapsed. The spectral shape in this range may be calculated only numerically from Eq. (4.86) with impact operator Tj, linear in n. Of course, it implies that binary theory is still valid and that vibrational dephasing is not yet... [Pg.193]

A schematic diagram of the experimental apparatus is shown in Fig. 1. A rotating fluidized bed composes of a plenum chamber and a porous cylindrical air distributor (ID400xD100mm) made of stainless sintered mesh with 20(xm openings [2-3]. The horizontal cylinder (air distributor) rotates around its axis of symmetry inside the plenum chamber. There is a stationary cylindrical filter (ID140xD100mm, 20(o.m openings) inside the air distributor to retain elutriated fine particle. A binary spray nozzle moimted on the metal filter sprays binder mist into the particle bed. A pulse air-jet nozzle is also placed inside the filter, which cleans up the filter surface in order to prevent clogging. [Pg.486]

If your molecule belongs to die group 0ooh> it also has an infinite number of binary axes of rotation and a center of inversion. Please check. [Pg.191]

You have replied that your molecule has a 5-fold axis of rotation. Verify that it also has 15 binary axes and ten ternary axes. Note that it belongs to one of the icosahedral groups. If you play soccer, consider the ball. Before you kick it, look at it. What is its symmetry ... [Pg.191]

Is there, then, an improper axis S(Note that if n > 2, the n-fold rotation axis C is by convention taken to be the vertical (z) axis). You have replied that there is indeed an axis Sjn. However, are there other binary axes perpendicular to the If not, the symmetry of your molecule is described by one of the groups Ja, (Note that if n is odd, there is a center of inversion). However, this result is subject to doubt, as there are very few molecules of symmetry J ... [Pg.401]


See other pages where Binary rotation is mentioned: [Pg.314]    [Pg.321]    [Pg.25]    [Pg.223]    [Pg.231]    [Pg.237]    [Pg.250]    [Pg.257]    [Pg.422]    [Pg.422]    [Pg.314]    [Pg.321]    [Pg.25]    [Pg.223]    [Pg.231]    [Pg.237]    [Pg.250]    [Pg.257]    [Pg.422]    [Pg.422]    [Pg.830]    [Pg.205]    [Pg.205]    [Pg.176]    [Pg.888]    [Pg.5]    [Pg.8]    [Pg.12]    [Pg.37]    [Pg.41]    [Pg.110]    [Pg.145]    [Pg.195]    [Pg.313]    [Pg.146]    [Pg.61]    [Pg.436]   
See also in sourсe #XX -- [ Pg.25 ]




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