Difference between revisions of "Projective determination of a metric"
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The concept of congruence of segments thus defined allows one to introduce a metric of a Euclidean space in $ E _ {n} $. | The concept of congruence of segments thus defined allows one to introduce a metric of a Euclidean space in $ E _ {n} $. | ||
For this, in the projective space $ P $ | For this, in the projective space $ P $ | ||
− | a system of [[Projective coordinates|projective coordinates]] is introduced with the basis simplex $ OA _ {1} | + | a system of [[Projective coordinates|projective coordinates]] is introduced with the basis simplex $ OA _ {1} \dots A _ {n} $, |
where the point $ O $ | where the point $ O $ | ||
does not not belong to the ideal hyperplane $ \pi $ | does not not belong to the ideal hyperplane $ \pi $ | ||
− | while the points $ A _ {1} \dots A _ {n} $ | + | while the points $ A _ {1}, \dots, A _ {n} $ |
do. Suppose that the point $ O $ | do. Suppose that the point $ O $ | ||
− | in this coordinate system has the coordinates $ 0 \dots 0 , 1 $, | + | in this coordinate system has the coordinates $ 0, \dots, 0 , 1 $, |
and that the points $ A _ {i} $, | and that the points $ A _ {i} $, | ||
− | $ i = 1 \dots n $, | + | $ i = 1, \dots, n $, |
have the coordinates | have the coordinates | ||
$$ | $$ | ||
− | x _ {1} = 0 \dots x _ {i-1} = 0 ,\ | + | x _ {1} = 0, \dots, x _ {i-1} = 0 ,\ |
x _ {i} = 1 , x _ {i+1} = 0, \dots, x _ {n+1} = 0 . | x _ {i} = 1 , x _ {i+1} = 0, \dots, x _ {n+1} = 0 . | ||
$$ | $$ | ||
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$$ | $$ | ||
u _ {i} = \sum _ { j= 1} ^ { n } a _ {ij} x _ {j} ,\ \ | u _ {i} = \sum _ { j= 1} ^ { n } a _ {ij} x _ {j} ,\ \ | ||
− | i = 1 \dots n . | + | i = 1, \dots, n . |
$$ | $$ | ||
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$$ | $$ | ||
− | Q ( x _ {1} \dots x _ {n} ) = \sum a _ {ij} x _ {i} x _ {j} $$ | + | Q ( x _ {1}, \dots, x _ {n} ) = \sum a _ {ij} x _ {i} x _ {j} $$ |
corresponding to it is positive definite. Let | corresponding to it is positive definite. Let | ||
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− | \frac{a _ 1}{a _ {n+1}} = x _ {1} \dots | + | \frac{a _ 1}{a _ {n+1}} = x _ {1}, \dots, |
\frac{a _ n}{a _ {n+ 1}} = x _ {n} ; | \frac{a _ n}{a _ {n+ 1}} = x _ {n} ; | ||
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− | \frac{b _ 1}{b _ {n+1}} = y _ {1} \dots | + | \frac{b _ 1}{b _ {n+1}} = y _ {1}, \dots, |
\frac{b _ n}{b _ {n+1}} = y _ {n} . | \frac{b _ n}{b _ {n+1}} = y _ {n} . | ||
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$$ | $$ | ||
− | \rho ( X , Y ) = \sqrt {Q ( x _ {1} - y _ {1} \dots x _ {n} - y _ {n} ) } . | + | \rho ( X , Y ) = \sqrt {Q ( x _ {1} - y _ {1}, \dots, x _ {n} - y _ {n} ) } . |
$$ | $$ | ||
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$$ | $$ | ||
− | X = ( x _ {1} : \dots : x _ {n+} | + | X = ( x _ {1} : \dots : x _ {n+1}) ,\ \ |
− | Y = ( y _ {1} : \dots : y _ {n+} | + | Y = ( y _ {1} : \dots : y _ {n+1}) , |
$$ | $$ | ||
Latest revision as of 10:04, 21 March 2022
An introduction in subsets of a projective space, by methods of projective geometry, of a metric such that these subsets become isomorphic to a Euclidean, hyperbolic or elliptic space. This is achieved by distinguishing in the class of all projective transformations (cf. Projective transformation) those transformations that generate in these subsets a group of transformations isomorphic to the corresponding group of motions. The presence of motions allows one "to lay off" segments of a straight line from a given point in a given direction, thereby introducing the concept of the length of a segment.
To obtain the Euclidean determination of a metric in the $ n $-dimensional projective space $ P $, one should distinguish in this space an $ ( n - 1 ) $-dimensional hyperplane $ \pi $, called the ideal hyperplane, and establish in this hyperplane an elliptic polar correspondence $ \Pi $ of points and $ ( n - 2 ) $-dimensional hyperplanes (that is, a polar correspondence under which no point belongs to the $ ( n - 2 ) $-dimensional plane corresponding to it).
Suppose that $ E _ {n} $ is a subset of the projective space $ P $ obtained by removing from it an ideal hyperplane; and let $ X, Y , X ^ \prime , Y ^ \prime $ be points in $ E _ {n} $. Two segments $ XY $ and $ X ^ \prime Y ^ \prime $ are said to be congruent if there exists a projective transformation $ \phi $ taking the points $ X $ and $ Y $ to the points $ X ^ \prime $ and $ Y ^ \prime $, respectively, and preserving the polarity $ \Pi $.
The concept of congruence of segments thus defined allows one to introduce a metric of a Euclidean space in $ E _ {n} $. For this, in the projective space $ P $ a system of projective coordinates is introduced with the basis simplex $ OA _ {1} \dots A _ {n} $, where the point $ O $ does not not belong to the ideal hyperplane $ \pi $ while the points $ A _ {1}, \dots, A _ {n} $ do. Suppose that the point $ O $ in this coordinate system has the coordinates $ 0, \dots, 0 , 1 $, and that the points $ A _ {i} $, $ i = 1, \dots, n $, have the coordinates
$$ x _ {1} = 0, \dots, x _ {i-1} = 0 ,\ x _ {i} = 1 , x _ {i+1} = 0, \dots, x _ {n+1} = 0 . $$
Then the elliptic polar correspondence $ \Pi $ defined in the hyperplane $ \pi $ can be written in the form
$$ u _ {i} = \sum _ { j= 1} ^ { n } a _ {ij} x _ {j} ,\ \ i = 1, \dots, n . $$
The matrix $ ( a _ {ij} ) $ of this correspondence is symmetric, and the quadratic form
$$ Q ( x _ {1}, \dots, x _ {n} ) = \sum a _ {ij} x _ {i} x _ {j} $$
corresponding to it is positive definite. Let
$$ X = ( a _ {1} : \dots : a _ {n+1} ) \ \ \textrm{ and } \ Y = ( b _ {1} : \dots : b _ {n+1} ) $$
be two points in $ E _ {n} $ (that is, $ a _ {n+1} \neq 0 $, $ b _ {n+1} \neq 0 $). One may set
$$ \frac{a _ 1}{a _ {n+1}} = x _ {1}, \dots, \frac{a _ n}{a _ {n+ 1}} = x _ {n} ; $$
$$ \frac{b _ 1}{b _ {n+1}} = y _ {1}, \dots, \frac{b _ n}{b _ {n+1}} = y _ {n} . $$
Then the distance $ \rho $ between the points $ X $ and $ Y $ is defined by
$$ \rho ( X , Y ) = \sqrt {Q ( x _ {1} - y _ {1}, \dots, x _ {n} - y _ {n} ) } . $$
For a projective determination of the metric of the $ n $-dimensional hyperbolic space, in the $ n $-dimensional projective space $ P $ a set $ U $ of interior points of a real oval hypersurface $ S $ of order two is considered. Let $ X , Y , X ^ \prime , Y ^ \prime $ be points in $ U $; then the segments $ XY $ and $ X ^ \prime Y ^ \prime $ are assumed to be congruent if there is a projective transformation of the space $ P $ under which the hypersurface $ S $ is mapped onto itself and the points $ X $ and $ Y $ are taken to the points $ X ^ \prime $ and $ Y ^ \prime $, respectively. The concept of congruence of segments thus introduced establishes in $ U $ the metric of the hyperbolic space. The length of a segment in this metric is defined by
$$ \rho ( X , Y ) = c | \mathop{\rm ln} ( XYPQ ) | , $$
where $ P $ and $ Q $ are the points of intersection of the straight line $ XY $ with the hypersurface $ S $ and $ c $ is a positive number related to the curvature of the Lobachevskii space. To introduce an elliptic metric in the projective space $ P $, one considers an elliptic polar correspondence $ \Pi $ in this space. Two segments $ XY $ and $ X ^ \prime Y ^ \prime $ are said to be congruent if there exists a projective transformation $ \phi $ taking the points $ X $ and $ Y $ to the points $ X ^ \prime $ and $ Y ^ \prime $, respectively, and preserving the polar mapping $ \Pi $ (that is, for any point $ M $ and its polar $ m $, the polar of the point $ \phi ( M) $ is $ \phi ( m) $). If the elliptic polar correspondence $ \Pi $ is given by the relations
$$ u _ {i} = \sum _ { j= 1} ^ { n+ 1} a _ {ij} x _ {j} ,\ \ i = 1, \dots, n + 1 , $$
then the matrix $ ( a _ {ij} ) $ is symmetric and the quadratic form corresponding to it is positive definite. Now, if
$$ X = ( x _ {1} : \dots : x _ {n+1}) ,\ \ Y = ( y _ {1} : \dots : y _ {n+1}) , $$
then
$$ \rho ( X , Y ) = \mathop{\rm arccos} \frac{| B ( X , Y ) | }{\sqrt {B ( X , X ) } \sqrt {B ( Y , Y ) } } , $$
where $ B $ is the bilinear form given by the matrix $ ( a _ {ij} ) $.
In all the cases considered (if a real projective space is completed to a complex projective space), under the projective transformations defining the congruence of segments, that is, under motions, some hypersurfaces of the second order remain invariant; these are called absolutes. In the case of a Euclidean determination of a metric, the absolute is an imaginary $ ( n - 2 ) $-dimensional oval surface of order two. In the case of a hyperbolic determination of a metric, the absolute is an oval $ ( n - 1 ) $-dimensional real hypersurface of order two. In the case of an elliptic determination of a metric, the absolute is an imaginary $ ( n - 1 ) $-dimensional oval hypersurface of order two.
References
[1] | N.V. Efimov, "Higher geometry" , MIR (1980) (Translated from Russian) |
[2] | N.A. Glagolev, "Projective geometry" , Moscow (1963) (In Russian) |
[3] | H. Busemann, P.J. Kelly, "Projective geometry and projective metrics" , Acad. Press (1953) |
Comments
References
[a1] | S. Kobayashi, "Transformation groups in differential geometry" , Springer (1972) |
Projective determination of a metric. Encyclopedia of Mathematics. URL: http://encyclopediaofmath.org/index.php?title=Projective_determination_of_a_metric&oldid=52249