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Grazing collision

Let us consider what we can learn about cross sections from some general considerations. Consider the reaction of an uncharged particle (a neutron) with a nucleus as shown in Figure 10.7. The neutron makes a grazing collision with the nucleus. The impact parameter b is taken to be the sum of the radii of the projectile and target nuclei. Thus, the cross section can be written as... [Pg.259]

Figure 10.7 Schematic diagram of a grazing collision of a neutron with a nucleus. Figure 10.7 Schematic diagram of a grazing collision of a neutron with a nucleus.
FIGURE 9.2 Relative speeds (RSs) of molecules for (a) head-on collision (RS = 2c), (b) grazing collision (RS = 0), and (c) right-angle collision (RS = fl c). For molecules moving in the same direction with the same velocity, the relative velocity of approach is zero. If they approach head-on, the relative velocity of approach is 2c. If they approach at 90°, the relative velocity of approach is the sum of the velocity components along the line. [Pg.398]

First came dust accretion to form the protoearth, a hot, dry rock. A grazing collision between the Earth and a Mars-sized body formed the moon. All volatile substances, including water, were lost. There is mounting evidence that comets could have provided the young Earth with its water, atmosphere, and carbon compounds that seeded prebiotic life (Delsemme, 2001 de Duve, 1995). But prebiotic Earth would have been much different from present-day Earth. [Pg.118]

Fig. 7.10 Shapes of droplets produced by an unstable (a) head-on and (b) grazing collision of two equal-sized water droplets in air, at Re = 2,500 and We = 38, as simulated by solving the Navier-Stokes equations, hi (b), the non-dimensional impact parameter X = 0.55 the non-dimensional time is defined as T = t UId [54] (Reprinted from [54], Copyright 1995, with permission from Elsevier)... Fig. 7.10 Shapes of droplets produced by an unstable (a) head-on and (b) grazing collision of two equal-sized water droplets in air, at Re = 2,500 and We = 38, as simulated by solving the Navier-Stokes equations, hi (b), the non-dimensional impact parameter X = 0.55 the non-dimensional time is defined as T = t UId [54] (Reprinted from [54], Copyright 1995, with permission from Elsevier)...
Fig. 7.11 Shapes of droplets produced by an unstable grazing collision of two equal-sized propanol-2 droplets in air at Re = 100 and We = 106 - (a) experiment, (b) lattice-Boltzmann simulation. The non-dimensional impact parameter X = 0.484 [63] (Reprinted with kind permission from Dr. Markus Schelkle, Immenstaad (Germany) 2010)... Fig. 7.11 Shapes of droplets produced by an unstable grazing collision of two equal-sized propanol-2 droplets in air at Re = 100 and We = 106 - (a) experiment, (b) lattice-Boltzmann simulation. The non-dimensional impact parameter X = 0.484 [63] (Reprinted with kind permission from Dr. Markus Schelkle, Immenstaad (Germany) 2010)...
Fig. 7.12 Shapes of droplets produced by a stable grazing collision of two equal-sized two-dimensional droplets at/fe f 31 and We 2. The non-dimensional impact parameterX = 0.5. The non-dimensional time t is the ratio of the dimensional time to the scale pd/2o [68] (Reprinted fiom [68], Copyright 2005, with permission from Elsevier)... Fig. 7.12 Shapes of droplets produced by a stable grazing collision of two equal-sized two-dimensional droplets at/fe f 31 and We 2. The non-dimensional impact parameterX = 0.5. The non-dimensional time t is the ratio of the dimensional time to the scale pd/2o [68] (Reprinted fiom [68], Copyright 2005, with permission from Elsevier)...
Kauftnann R, Wolfgang R (1959) Complex nucleon transfer reaction of heavy ions. Phys Rev Lett 3 232 Kauftnann R, Wolfgang R (1961) Nucleon transfer reactions in grazing collisions of heavy ions. Phys Rev... [Pg.34]

Translational Energy Spectrum (TES). In the high-resolution TES recorded from grazing collisions of a fast NH ion beam with He as the neutral target gas, two inelastic peaks at energy losses of 2.7 and 4.1 eV were observed and assigned to the A Z"<<-X and C Z X 11 transitions of NH" the peak at 4.1 eV showed partially resolved vibrational structure (AEj O.35 eV 2800 cm" ) of the ground state [22]. [Pg.148]

Fig. 2. Absorption spectrum and time dependence for the model of ICN photodissociation of reference 8. If we cut off the time interval of the Fourier transform in equation (8) to (-Tq,Tq), we obtain the smooth envelope (dashed line) of the structured spectrum. The structure is caused by a "grazing collision" of < (t) with Fig. 2. Absorption spectrum and time dependence for the model of ICN photodissociation of reference 8. If we cut off the time interval of the Fourier transform in equation (8) to (-Tq,Tq), we obtain the smooth envelope (dashed line) of the structured spectrum. The structure is caused by a "grazing collision" of < (t) with <j) (near Tj) as < )(t) dissociates. The method used is the second discussed in section 4.

See other pages where Grazing collision is mentioned: [Pg.1308]    [Pg.132]    [Pg.331]    [Pg.279]    [Pg.280]    [Pg.280]    [Pg.121]    [Pg.207]    [Pg.471]    [Pg.203]    [Pg.169]    [Pg.1308]    [Pg.455]    [Pg.31]    [Pg.132]    [Pg.161]    [Pg.170]    [Pg.171]    [Pg.172]    [Pg.173]    [Pg.175]    [Pg.353]    [Pg.666]    [Pg.358]    [Pg.206]    [Pg.638]    [Pg.376]    [Pg.117]    [Pg.711]   
See also in sourсe #XX -- [ Pg.114 ]




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