Abstract Generated abstract
The paper studies the relation between four-dimensional symmetric conformally Euclidean spaces of zero signature and line geometries associated with subgroups of projective transformations of three-dimensional projective space. It introduces generalized biplanar spaces defined by absolute collineations and classifies their associated B-quadrics in the hyperbolic, elliptic, and parabolic cases by reducing the relevant matrices to canonical forms and identifying invariants. Using the realization of symmetric conformally Euclidean spaces as internal geometries of normalized B-quadrics and the Plücker representation of lines, the paper derives a classification of projective subgroups whose line geometries determine such symmetric spaces. The resulting table links types of B-quadric envelopes with corresponding conformally Euclidean spaces and with symplectic, elliptic, hyperbolic, Euclidean, pseudo-Euclidean, and related line geometries.
Full Text
V. D. Tretyakov
On the Question of Line Geometry in Three-Dimensional Klein Spaces
(Presented by Academician A. I. Mal’tsev on 27 IV 1963)
In the present paper a correspondence is established between symmetric conformally Euclidean spaces ($SC$-spaces) of four dimensions and zero signature and the line geometries of various subgroups of projective transformations of three-dimensional space.
- Consider the collineation
\[ \tilde{x}^{\alpha}=\gamma_{\sigma}^{\alpha}x^{\sigma} \qquad (\alpha,\beta,\ldots,\sigma=1,2,\ldots,n+2); \tag{1} \]
in the projective space \(P_{n+1}\), satisfying the condition
\[ \gamma_{\sigma}^{\alpha}\gamma_{\beta}^{\sigma}=\varepsilon\delta_{\beta}^{\alpha} \qquad (\varepsilon=\pm1,\;0). \tag{2} \]
We shall call this collineation absolute.
The generalized biplanar space \(B_{n+1}\) is the \((n+1)\)-dimensional space whose fundamental group is isomorphic to the subgroup of projective transformations taking the absolute collineation (1) into itself.
For \(\varepsilon=1\) (hyperbolic \(B_{n+1}\)) the absolute collineation is a projective symmetry in an \(m\)-pair; the case \(\varepsilon=-1\) is possible only in a space of an odd number of dimensions (elliptic \(B_{2k+1}\)) and corresponds to a biplanar involution of elliptic type; for \(\varepsilon=0\) (parabolic \(B_{n+1}\)) the matrix \((\gamma_{\beta}^{\alpha})\) is a nilpotent matrix of general form \(({}^{6},\ p.\ 16)\).
A \(B\)-quadric \(Q_n\) of the generalized biplanar space \(B_{n+1}\) is called \(({}^{6},\ p.\ 17)\) a quadric \(Q_n\), \(a_{\alpha\beta}x^{\alpha}x^{\beta}=0\), defined by a symmetric tensor \(a_{\alpha\beta}\), for which the tensor adjoint to it \(({}^{2},\ p.\ 145)\)
\[ b_{\alpha\beta}=a_{\alpha\sigma}\gamma_{\beta}^{\sigma} \tag{3} \]
is also symmetric.
The absolute planes of the collineation (1) are polar conjugate with respect to the \(B\)-quadric in the elliptic and hyperbolic cases and belong to it in the parabolic case.
- B. A. Rosenfeld has proved \(({}^{3},\ p.\ 368)\) that the groups of motions of the spaces of constant curvature \(S_3\), \({}^{1}S_3\), and \({}^{2}S_3\) are isomorphic to subgroups of motions of the space \({}^{3}S_5\) leaving fixed two planes that are polar conjugate with respect to the absolute, i.e., taking into themselves certain involutions in \(P_5\). Thus, these groups are isomorphic to subgroups of biplanar motions preserving the polarity induced by the \(B\)-quadric. It is not difficult to show that the groups of motions of the Euclidean \(R_3\) and pseudo-Euclidean \({}^{1}R_3\) spaces are isomorphic to subgroups of motions of a biplanar space of parabolic type, preserving a \(B\)-polarity.
In connection with this there arises the question of classifying \(B\)-quadrics and establishing a correspondence between their types and the line geometries of three-dimensional spaces.
- We shall carry out the classification of \(B\)-quadrics separately for each of the three types \(B_{n+1}\).
A. Hyperbolic type: \(\gamma_\sigma^\alpha \gamma_\beta^\sigma=\delta_\beta^\alpha\). The matrices of the absolute involution \((\gamma_\beta^\alpha)\), of the \(B\)-quadric \((a_{\alpha\beta})\), and of the \(B\)-motion \((t_\beta^\alpha)\) are reduced to the form:
\[ (\gamma_\beta^\alpha)= \begin{pmatrix} -E_{m+1} & 0\\ 0 & E_{n-m+1} \end{pmatrix}; \qquad (a_{\alpha\beta})= \begin{pmatrix} -E_p & & \\ & E_r & 0\\ & 0 & -E_q\\ & & E_s \end{pmatrix}; \qquad (t_\beta^\alpha)= \begin{pmatrix} P_{m+1} & 0\\ 0 & Q_{n-m+1} \end{pmatrix}, \]
where \(E_i\) is the identity matrix of order \(i\); \(P_{m+1}\) and \(Q_{n-m+1}\) are arbitrary (square) matrices. The numbers \(p,q,r,s\) are related by the relations \(p+r=m+1\), \(q+s=n-m+1\). The index \(l\) ([3], p. 297) of the \(B\)-quadric is equal to \(l=p+q\). If \(m=n/2\) (\(n\) even), one can arrange that \(p>q\).
The numbers \(p,q\), and \(m\) form a complete system of invariants of the \(B\)-quadric. If \(n=2k,\ m=k\) (the proper biplanar space), one can introduce a canonical coordinate system in which
\[ (\gamma_\beta^\alpha)= \begin{pmatrix} 0 & E\\ E & 0 \end{pmatrix}. \]
In this case the matrix of a \(B\)-quadric of zero signature can be reduced to the form
\[ (a_{\alpha\beta})= \begin{pmatrix} 0 & C\\ C & 0 \end{pmatrix}; \qquad C= \begin{pmatrix} E_p & 0\\ 0 & E_{k-p+1} \end{pmatrix}. \tag{4} \]
Generally speaking, in this case, in the canonical coordinate system the matrix of a \(B\)-quadric cannot be reduced either to the form (4) or to diagonal form (the latter is possible when \(p=q\)).
B. Elliptic type: \(\gamma_\sigma^\alpha\gamma_\beta^\sigma=-\delta_\beta^\alpha\). The matrices \((\gamma_\beta^\alpha)\), \((a_{\alpha\beta})\), and \((t_\beta^\alpha)\) are reduced to the form:
\[ (\gamma_\beta^\alpha)= \begin{pmatrix} 0 & -E_{k+1}\\ E_{k+1} & 0 \end{pmatrix}; \qquad (a_{\alpha\beta})= \begin{pmatrix} 0 & E_{k+1}\\ E_{k+1} & 0 \end{pmatrix}; \qquad (t_\beta^\alpha)= \begin{pmatrix} P_{k+1} & -Q_{k+1}\\ Q_{k+2} & P_{k+1} \end{pmatrix} \]
(cf. ([1], p. 93)).
C. Parabolic type: \(\gamma_\alpha^\sigma\gamma_\sigma^\beta=0\). The matrices \((\gamma_\beta^\alpha)\), \((a_{\alpha\beta})\), and \((t_\beta^\alpha)\) are reduced to the form
\[ (\gamma_\beta^\alpha)= \begin{pmatrix} 0 & 0 & 0\\ E_r & 0 & 0\\ 0 & 0 & 0 \end{pmatrix}; \qquad (a_{\alpha\beta})= \begin{pmatrix} 0 & C_r & 0\\ C_r & 0 & 0\\ 0 & 0 & B_s \end{pmatrix}; \qquad (t_\beta^\alpha)= \begin{pmatrix} P_r & 0 & 0\\ Q_r & P_r & T\\ S & 0 & R_s \end{pmatrix}; \]
\[ C_r= \begin{pmatrix} -E_k & 0\\ 0 & E_{r-k} \end{pmatrix}; \qquad B_s= \begin{pmatrix} -E_l & 0\\ 0 & E_{s-l} \end{pmatrix}; \]
\(P_r,Q_r,R_s\) are square matrices, and \(S\) and \(T\) are arbitrary rectangular matrices.
A \(B\)-quadric of zero signature exists in \(B_{2n+1}\) in any of the indicated cases; moreover, if the matrix of the absolute collineation is changed in the corresponding manner, the matrix of the \(B\)-quadric will have the form
\[ \begin{pmatrix} 0 & E\\ E & 0 \end{pmatrix}. \]
The results obtained make it possible to carry out a classification of the subgroups of biplanar motions that leave invariant the polarity determined by the given \(B\)-quadric.
- A. P. Shirokov ([6]) proved that the geometry of any symmetric conformally Euclidean space (an \(SC\)-space) can be realized as the internal geometry of a \(B\)-quadric normalized by means of an absolute involution.
Since the transformation group \(P_5\) leaving invariant the Plücker hyperquadric \(Q_4\) is isomorphic to the group of projective transformations in \(P_3\), the classification of \(B\)-motions leaving \(Q_4\) invariant makes it possible to distinguish all subgroups of projective transformations of three-dimensional space whose line geometries, under the mapping onto the Plücker hyperquadric, determine a symmetric space.
As a result we obtain Table 1. Cases 4–8 of this table correspond to the spaces considered by A. P. Norden ([2], p. 153). Clas-
Table 1
| Type of envelope in \(P_5\) | No. | Additional data | Type of \({}^2SC_4\), dimension and characteristic in the completely geodesic case of reducibility | Type of three-dimensional space whose line geometry is realized in \({}^2SC_4\) |
|---|---|---|---|---|
| Hyperbolic | 1 | \(m=0\) | Of constant curvature | Symplectic |
| Hyperbolic | 2 | \(m=1\) \(p=1\) |
Reducible, i.e., three-dimensional; the family, i.e., does not contain isotropic surfaces | Biaxial of elliptic type |
| Hyperbolic | 3 | \(m=1\) \(p=2\) |
Reducible, i.e., three-dimensional; the family, i.e., contains 2 isotropic surfaces | Biaxial of hyperbolic type |
| Hyperbolic | 4 | \(m=2\) \(p=2\) |
Reducible, i.e., two-dimensional hyperbolic spaces | Space with a line absolute |
| Hyperbolic | 5 | \(m=2\) \(p=3\) |
Reducible, i.e., two-dimensional elliptic spaces | Elliptic |
| Elliptic | 6 | — | Irreducible | Hyperbolic |
| Parabolic | 7 | \(r=3\) \(k=0\) |
Irreducible, type I | Euclidean |
| Parabolic | 8 | \(r=3\) \(k=1\) |
Irreducible, type II | Pseudo-Euclidean |
| Parabolic | 9 | \(r=2\) \(k=0\) |
Irreducible, type III | Absolute, decomposes into 2 imaginary straight lines |
| Parabolic | 10 | \(r=2\) \(k=1\) |
Irreducible, type IV | Absolute, decomposes into 2 real straight lines |
| Parabolic | 11 | \(r=1\) | Of zero curvature | Absolute, 2 coincident straight lines |
sification of \(SC\)-spaces agrees with the results of P. A. Shirokov \((^7)\). To the line geometry of all the spaces indicated in the last column of Table 1, the results of the work \((^4)\) are applicable. Using the projective interpretation of \(SC\)-spaces given by A. P. Shirokov \((^6)\), it is not difficult to construct a conformal interpretation of all these line geometries.
In this case the absolute invariant of two adjacent straight lines is determined by the quadratic form:
\[ g_{ij}=\partial_i x\,\partial_j x \qquad (i,j=1,\ldots,4), \]
where, as usual, \(xy=a_{\alpha\beta}x^\alpha x^\beta\) \((\alpha,\beta=1,\ldots,6)\), and the normalization of the points (straight lines) \(x\) is subject to the condition \(xx=1\) (see \((^4)\) and \((^6)\), p. 17).
Kuibyshev State
Pedagogical Institute
Received
21 IV 1963
CITED LITERATURE
\(^1\) G. E. Izotov, Izv. vyssh. uchebn. zaved., Matematika, No. 1 (2), 89 (1958).
\(^2\) A. P. Norden, Izv. vyssh. uchebn. zaved., Matematika, No. 4 (17), 145 (1960).
\(^3\) B. A. Rozenfeld, Non-Euclidean Geometries, 1957.
\(^4\) V. D. Tretyakov, Volzhskii Mat. Sborn., No. 1 (1963).
\(^5\) A. P. Shirokov, Uch. zap. Kazansk. gos. univ., 114, book 2 (1954).
\(^6\) A. P. Shirokov, Uch. zap. Kazansk. gos. univ., 116, book 1, 15 (1956).
\(^7\) P. A. Shirokov, Izv. Kazansk. fiz.-matem. obshch., 11, ser. 3, 9 (1938).