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Point at infinity

The Point at Infinity. In many problems we wish to find solutions of differential equations of the type (3.1) which are valid for large values of a . We seek solutions in... [Pg.9]

Wc consider first the solution corresponding to the singular point at infinity. We write... [Pg.62]

The particle density in an isolated bounded system is required to be zero at the boundary point at infinity. This introduces gaps (or discreteness) in the excitation spectrum, at low energy, which are not present in extended systems. The presence of shell structure, and whether the shells are open or closed, is... [Pg.36]

As we have shown, if a scalar field cf>(r) is one-valued at infinity (i.e. if its limit when r oc does not depend on the direction), it can be interpreted as a map (j) 53 f->52. To do that, one must identify, via stereographic projection, the 3-space plus the point at infinity R3 U oo with S3, and the complete complex plane C U oo with the sphere S2. [Pg.206]

For 5 = 0 (limit point at infinity), one obtains the corresponding Coulomb modifications, see Refs. [36,42] for the complications at origin. Note also the strong dependence on the incident directions for "ellipsoidal" potentials yet the optical theorem holds, see Ref. [39]. [Pg.44]

Any straight line with an extra point at infinity may be considered a circle with infinite radius. [Pg.219]

As it views a scene the eye does not respond directly to the objects in the scene, but to light rays that travel along straight lines from points in the scene to the eye. It follows that radial lines will look like points and radial planes look like lines. As a result radial dimensions are lost. A further consequence is that non-radial lines acquire an extra point at infinity. As shown in figure 11 the non-radial line L is observed through a set of radial lines in the plane OL. Only one radial line in OL does not connect a point on L to the eye. That one exception is the radial line parallel to L. This line Pqo appears to the eye as a point at infinity on L. The two parallel lines that meet at infinity are considered to intersect at an angle of zero. [Pg.239]

Figure 7.11 Point at infinity generated in perspective geometry. Figure 7.11 Point at infinity generated in perspective geometry.
Dirichlet function, which is an approximation of Delta function, S x). Various approximate representations of Dirac delta function are provided in Van der Pol Bremmer (1959) on pp 61-62. This clearly shows that we recover the applied boundary condition at y = 0. Therefore, the delta function is totally supported by the point at infinity in the wave number space (which is nothing but the circular arc of Fig. 2.20 i.e. the essential singularity of the kernel of the contour integral). [Pg.89]

It has already been explained that the eigenvalues near a = 0 gives rise to asymptotic solution, while the local solution is contributed by the point at infinity in the spectral plane a —> oo) (Sengupta Rao, 2006). Also, for small values of T and large values of b, the receptivity problem can be solved by linearizing the Navier -Stokes equation. [Pg.116]

Also interesting is the dynamical behavior associated with the fixed point at infinity, that is, q,p) = (oo,0). Here we introduce the concept of homoclinic orbit, which is a trajectory that goes to an unstable fixed point in the past as well as in the future. A homoclinic orbit thus passes the intersection between the unstable and stable manifolds of a particular fixed point. Indeed, as shown in Fig. 6, these manifolds generate a so-called homoclinic web. In particular. Fig. 6a displays a Smale horseshoe giving a two-symbol subdynamics, indicating that the fixed point (oo,0) is not a saddle. Nevertheless, it is stUl unstable with distinct stable and unstable manifolds, with its dynamics much slower than that for a saddle. Figure 6b shows an example of a numerical plot of the stable and unstable manifolds. [Pg.24]

Note that we have derived the Kirchhoff formula (13.112) only for bounded domains. Equipped now with the radiation conditions, we can apply this formula to unbounded domains as well. Let us consider a domain V, which may include a point at infinity. The domain V is bounded by the surface S (Figure 13-4). [Pg.434]

The mountain-pass theorem describes how to find the critical point x in a path between two points, Xa and Xb oi a given n-dimensional function, /. The critical point being that point which must he on the best pathway between two points, and x More and Munson describes the mountain-pass theorem in it s most basic form, stating that the mountain-pass theorem shows that if x G i-> M, and / has no critical points at infinity, then the critical point, x. in the path between Xaand Xb GW with /(x ) < /fxj, is such that the value of / at x is given by... [Pg.482]

As a rule, the region occupied by a moving reactive mixture is not the entire space but only a part bounded by some surfaces. According to whether the point at infinity belongs to the flow region or not, the problem of finding the unknown functions is called the exterior or interior problem of hydrodynamics, respectively. [Pg.4]

The key observation is that Levi-Civita s conformal map (7), u i—> x = u2, not only regularizes collisions at x = 0 but also analogous singularities at x = oo. This is seen by closing the complex planes to become Riemann spheres (by adding the point at infinity) and using inversions x = 1/x, u = 1/u. [Pg.246]

The original motivation for introducing Pn(k) was to add to the affine space kn = Uq the extra points at infinity Pn k) — Uo so as to bring out into the open the mysterious things that went on at infinity. [Pg.8]

Recall that to all subvectorspaces W C kn+1 one associates the set of points P e Pn(k) with homogeneous coordinates in W the sets so obtained are called the linear subspaces L of Pn(fc). If W has codimension 1, then we get a hyperplane. In particular, the points at infinity with respect to the affine piece Ui form the hyperplane associated to the subvectorspace Xi = 0. Moreover, by introducing a basis into W, the linear subspace L associated to W is naturally isomorphic to Pr(k), (r = dim W — 1). The linear subspaces are the simplest examples of projective algebraic sets ... [Pg.8]


See other pages where Point at infinity is mentioned: [Pg.822]    [Pg.9]    [Pg.9]    [Pg.10]    [Pg.16]    [Pg.24]    [Pg.25]    [Pg.301]    [Pg.301]    [Pg.303]    [Pg.335]    [Pg.4]    [Pg.201]    [Pg.236]    [Pg.240]    [Pg.44]    [Pg.354]    [Pg.217]    [Pg.229]    [Pg.240]    [Pg.241]    [Pg.6]    [Pg.331]    [Pg.426]    [Pg.426]    [Pg.33]    [Pg.161]    [Pg.426]    [Pg.426]    [Pg.402]   
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See also in sourсe #XX -- [ Pg.239 ]

See also in sourсe #XX -- [ Pg.55 , Pg.231 , Pg.305 ]




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