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Difference between revisions of "Projective determination of a metric"

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An introduction in subsets of a [[Projective space|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|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.
 
An introduction in subsets of a [[Projective space|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|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 $-
+
To obtain the Euclidean determination of a metric in the  $  n $-dimensional projective space  $  P $,  
dimensional projective space  $  P $,  
+
one should distinguish in this space an  $  ( n - 1 ) $-dimensional hyperplane  $  \pi $,  
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 $
 
called the ideal hyperplane, and establish in this hyperplane an elliptic polar correspondence  $  \Pi $
of points and  $  ( n - 2 ) $-
+
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).
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} $
 
Suppose that  $  E _ {n} $
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$$  
 
$$  
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 .
 
$$
 
$$
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$$  
 
$$  
X  =  ( a _ {1} : \dots : a _ {n+} 1 ) \ \  
+
X  =  ( a _ {1} : \dots : a _ {n+1} ) \ \  
\textrm{ and } \  Y  =  ( b _ {1} : \dots : b _ {n+} 1 )
+
\textrm{ and } \  Y  =  ( b _ {1} : \dots : b _ {n+1} )
 
$$
 
$$
  
be two points in  $  E _ {n} $(
+
be two points in  $  E _ {n} $ (that is,  $  a _ {n+1} \neq 0 $, $  b _ {n+1} \neq 0 $).  
that is,  $  a _ {n+} 1 \neq 0 $,  
 
$  b _ {n+} 1 \neq 0 $).  
 
 
One may set
 
One may set
  
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\frac{a _ 1}{a _ n+}
+
\frac{a _ 1}{a _ {n+1}}  =  x _ {1} \dots  
  1 =  x _ {1} \dots  
 
 
 
\frac{a _ n}{a _ n+}
+
\frac{a _ n}{a _ {n+ 1}}  =  x _ {n} ;
  1 =  x _ {n} ;
 
 
$$
 
$$
  
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\frac{b _ 1}{b _ n+}
+
\frac{b _ 1}{b _ {n+1}}  =  y _ {1} \dots  
  1 =  y _ {1} \dots  
 
 
 
\frac{b _ n}{b _ n+}
+
\frac{b _ n}{b _ {n+1}}  =  y _ {n} .
  1 =  y _ {n} .
 
 
$$
 
$$
  
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$$
 
$$
  
For a projective determination of the metric of the  $  n $-
+
For a projective determination of the metric of the  $  n $-dimensional hyperbolic space, in the  $  n $-dimensional projective space  $  P $
dimensional hyperbolic space, in the  $  n $-
 
dimensional projective space  $  P $
 
 
a set  $  U $
 
a set  $  U $
 
of interior points of a real oval hypersurface  $  S $
 
of interior points of a real oval hypersurface  $  S $
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to the points  $  X  ^  \prime  $
 
to the points  $  X  ^  \prime  $
 
and  $  Y  ^  \prime  $,  
 
and  $  Y  ^  \prime  $,  
respectively, and preserving the polar mapping  $  \Pi $(
+
respectively, and preserving the polar mapping  $  \Pi $ (that is, for any point  $  M $
that is, for any point  $  M $
 
 
and its polar  $  m $,  
 
and its polar  $  m $,  
 
the polar of the point  $  \phi ( M) $
 
the polar of the point  $  \phi ( M) $
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$$  
 
$$  
u _ {i}  =  \sum _ { j= } 1 ^ { n+ } 1 a _ {ij} x _ {j} ,\ \  
+
u _ {i}  =  \sum _ { j= 1} ^ { n+ 1} a _ {ij} x _ {j} ,\ \  
i = 1 \dots n + 1 ,
+
i = 1, \dots, n + 1 ,
 
$$
 
$$
  
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is the bilinear form given by the matrix  $  ( a _ {ij} ) $.
 
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 ) $-
+
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.
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====
 
====References====

Revision as of 10:02, 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)
How to Cite This Entry:
Projective determination of a metric. Encyclopedia of Mathematics. URL: http://encyclopediaofmath.org/index.php?title=Projective_determination_of_a_metric&oldid=52249
This article was adapted from an original article by P.S. ModenovA.S. Parkhomenko (originator), which appeared in Encyclopedia of Mathematics - ISBN 1402006098. See original article