グラスマン多様体とその商空間の極大対蹠 集合
Antipodal sets of Grassmann
manifolds and their quotient spaces
田中 真紀子(東京理科大学)
第
2
回水戸幾何小研究集会2019
年6
月22
日–6
月23
日茨城大学
Joint work with Hiroyuki Tasaki.
1. Antipodal sets and 2-numbers
2. Maximal antipodal sets of Grassmann manifolds (1)
3. Maximal antipodal sets of Grassmann manifolds (2)
4. The quotient space G m ( K 2 m ) ∗ ( K = R , C , H ) 5. Maximal antipodal sets of G m ( K 2 m ) ∗
6. The 2-number and great antipodal sets
of G m ( K 2 m ) ∗
1. Antipodal sets and 2-numbers
M : compact Riemann symmetric space s x : geodesic symmetry at x
i.e., (i) s x is an isometry of M , (ii) s x 2 = id, (iii) x is an isolated fixed point of s x
S ⊂ M : subset
S : antipodal set ⇐⇒ ∀ def x, y ∈ S, s x ( y ) = y 2-number of M
# 2 M := max {| S | | S ⊂ M antipodal set }
S : great antipodal set ⇐⇒ | def S | = # 2 M
(Chen-Nagano 1988)
Examples. (1) M = S n ( ⊂ R n +1 )
{ x, − x } ( x ∈ S n ) : great antipodal set
# 2 S n = 2
(2) M = R P n
e 1 , . . . , e n +1
:o.n.b. of R n +1
{⟨ e 1 ⟩ R , . . . , ⟨ e n +1 ⟩ R } : great antipodal set
# 2 R P n = n + 1
(3) M = U ( n ) s x ( y ) = xy − 1 x
s 1
n( y ) = y ⇔ y 2 = 1 n (1 n : identity matrix)
x 2 = y 2 = 1 n ⇒ s x ( y ) = y iff xy = yx
∆ n :=
± 1
. . .
± 1
: great antipodal set
# 2 U ( n ) = 2 n
Theorem 1. (T.-Tasaki 2013) M : symmetric R -space
(1) Any antipodal set of M is included in a great antipodal set.
(2) Any two great antipodal sets are I 0 ( M )-
congruent.
I 0 ( M ) : identity component of I ( M ), the group of isometries of M
(3) A great antipodal set of M is an orbit of the Weyl group.
S n , R P n and U ( n ) are symmetric R -spaces.
A maximal antipodal set is not necessarily
a great antipodal set.
2. Maximal antipodal sets of Grassmann manifolds (1)
O ( n, K ) :=
O ( n ) ( K = R ) U ( n ) ( K = C ) Sp ( n ) ( K = H )
G m ( K n ) : Grassmann manifold of m -dim K - subspaces of K n
O ( n, K ) y G m ( K n ) transitively
G m ( K n ) = ∼ O ( n, K ) /O ( m, K ) × O ( n − m, K )
G m ( K n ) is a Riemann symmetric space w.r.t.
O ( n, K )-invariant Riemann metric. G m ( K n )
is a symmetric R -space.
x ∈ G m ( K n )
π x , π x
⊥:orthogonal projection onto x, x ⊥ ρ x := π x − π x
⊥: K n → K n
s x ( y ) = ρ x ( y ) ( y ∈ G m ( K n )) e 1 , . . . , e n : o.n.b. of K n
ρ e
i( e i ) = e i , ρ e
i( e j ) = − e j ( i ̸ = j ) s ⟨ e
i1
,...,e
im⟩
K( ⟨ e j
1, . . . , e j
m⟩ K ) = ⟨ e j
1, . . . , e j
m⟩ K
A := {⟨ e i
1, . . . , e i
m⟩ K | 1 ≤ i 1 < · · · < i m ≤ n } is an antipodal set of G m ( K n ).
| A | =
(
n m
)
= # 2 G m ( K n ) (Chen-Nagano)
A is a unique great antipodal set up to
I 0 ( G m ( K n ))-congruence by Theorem 1.
3. Maximal antipodal sets of Grassmann manifolds (2)
O ( n, K ) is a Riemann symmetric space w.r.t.
a bi-invariant metric.
x ∈ O ( n, K ), s x ( y ) = xy − 1 x ( y ∈ O ( n, K ))
1 n : identity matrix, s 1
n( y ) = y ⇔ y 2 = 1 n F ( s 1
n, O ( n, K )) =
∪0 ≤ k ≤ n
∪
g ∈ O ( n, K )
g
1 k
− 1 n − k
g − 1 ι : G m ( K n ) ∋ x 7→ ρ x ∈ O ( n, K ) : embedding
F ( s 1
n, O ( n, K )) =
∪0 ≤ k ≤ n
ι ( G k ( K n ))
G : compact Lie group, e : identity element G 0 : identity component of G
M : connected component of F ( s e , G ) M is a polar of G w.r.t. e .
x ∈ M, M = { I g ( x ) | g ∈ G 0 } , I g ( x ) = gxg − 1 I 0 ( M ) = { I g | M | g ∈ G 0 }
ι ( G m ( K n )) =
id G m ( K n ) is a polar of O ( n, K ) w.r.t. 1 n .
A : maximal antipodal set of G m ( K n )
{ 1 n } ∪ A : antipodal set of O ( n, K )
∃ A ˜ : maximal antipodal subgroup of O ( n, K ) s.t. { 1 n } ∪ A ⊂ A ˜
∃ g ∈ O ( n, K ) s.t. A ˜ = g ∆ n g − 1
When K = R , we can take g ∈ SO ( n ).
A = ˜ A ∩ G m ( K n )
A = g ∆ n g − 1 ∩ G m ( K n ) = g (∆ n ∩ G m ( K n )) g − 1
∆ n ∩ G m ( K n )
= ∆ m n :=
ε 1
. . .
ε n
∈ ∆ n
|{ i | ε i = 1 }| = m
A = g ∆ m n g − 1
∆ m n is a unique maximal antipodal set (hence a unique great antipodal set) of G m ( K n ) up to I 0 ( G m ( K n ))-congruence.
| ∆ m n | =
(
n m
)
= # 2 G m ( K n ) ι − 1 (∆ k n )
= {⟨ e i
1, . . . , e i
m⟩ K | 1 ≤ i 1 < · · · < i m ≤ n }
4. The quotient space G m ( K 2 m ) ∗ ( K = R , C , H ) γ : G m ( K 2 m ) ∋ x 7→ x ⊥ ∈ G m ( K 2 m ) : isometry
G m ( K 2 m ) ∗ := G m ( K 2 m ) / { id , γ }
s [ x ] ([ y ]) = [ s x ( y )] ([ x ] , [ y ] ∈ G m ( K 2 m ) ∗ ) O (2 m, K ) ∗ := O (2 m, K ) / {± 1 2 m }
π 2 m : O (2 m, K ) → O (2 m, K ) ∗ : projection
ι ◦ γ ( x ) = ι ( x ⊥ ) = ρ x
⊥= − ρ x ( x ∈ G m ( K 2 m )) G m ( K 2 m ) ∗ =
id ι ( G m ( K n )) / {± 1 2 m } ⊂ O (2 m, K ) ∗
G m ( K 2 m ) ∗ is a polar of O (2 m, K ) ∗ w.r.t. π 2 m (1 2 m ).
5. Maximal antipodal sets of G m ( K 2 m ) ∗ D [4] :=
± 1 0 0 ± 1
,
0 ± 1
± 1 0
n = 2 k · l, l : odd 0 ≤ s ≤ k
D ( s, n ) := D [4] ⊗ · · · ⊗ D [4]
| {z }
s
⊗ ∆ n/ 2
s⊂ O ( n )
= { d 1 ⊗ · · · ⊗ d s ⊗ d 0
| d 1 , . . . , d s ∈ D [4] , d 0 ∈ ∆ n/ 2
s}
∆ 2 ( D [4]
D ( k − 1 , 2 k ) = D [4] ⊗ · · · ⊗ D [4]
| {z }
k − 1
⊗ ∆ 2 ( D [4] ⊗ · · · ⊗ D [4]
| {z }
k − 1
⊗ D [4] = D ( k, 2 k )
Theorem 2. (T.-Tasaki 2017)
A maximal antipodal subgroup (MAS) of O ( n, K ) ∗ is given as follows.
(1) K = R . MAS of O ( n ) ∗ is O ( n ) ∗ -conjugate to one of the following.
π n ( D ( s, n )) (0 ≤ s ≤ k ) ,
where the case ( s, n ) = ( k − 1 , 2 k ) is excluded.
(2) K = C . MAS of U ( n ) ∗ is U ( n ) ∗ -conjugate to one of the following.
π n ( { 1 , √
− 1 } D ( s, n )) (0 ≤ s ≤ k ) ,
where the case ( s, n ) = ( k − 1 , 2 k ) is excluded.
(3) K = H . MAS of Sp ( n ) ∗ is Sp ( n ) ∗ -conjugate to one of the following.
π n ( { 1 , i , j , k } D ( s, n )) (0 ≤ s ≤ k ) ,
where the case ( s, n ) = ( k − 1 , 2 k ) is excluded.
In (1) we can replace “ O ( n ) ∗ -conjugate” by
“ SO ( n ) ∗ -conjugate”.
A : maximal antipodal set of G m ( K 2 m ) ∗
{ π 2 m (1 2 m ) } ∪ A : antipodal set of O (2 m, K ) ∗
∃ A ˜ : maximal antipodal subgroup of O (2 m, K ) ∗
s.t. { π 2 m (1 2 m ) } ∪ A ⊂ A ˜
A = ˜ A ∩ G m ( K 2 m ) ∗ 2 m = 2 k · l, l : odd Γ K :=
{ 1 } ( K = R ) { 1 , √
− 1 } ( K = C ) { 1 , i , j , k } ( K = H )
∃ g ∈ O (2 m, K ) ( ∃ g ∈ SO (2 m ) when K = R ) ,
∃ s ∈ { 0 , . . . , k } s.t.
A ˜ = π 2 m ( g ) π 2 m (Γ K D ( s, 2 m )) π 2 m ( g ) − 1
A = π 2 m ( g ) π 2 m (Γ K D ( s, 2 m )) π 2 m ( g ) − 1 ∩ G m ( K 2 m ) ∗
= π 2 m ( g ) π 2 m (Γ K D ( s, 2 m ) ∩ G m ( K 2 m )) π 2 m ( g ) − 1
P D ( s, 2 m ) := { d ∈ D ( s, 2 m ) | d 2 = 1 2 m }
N D ( s, 2 m ) := { d ∈ D ( s, 2 m ) | d 2 = − 1 2 m } D ( s, 2 m ) ∩ G m ( R 2 m )
= { d ∈ D ( s, 2 m ) | d 2 = 1 2 m , Tr d = 0 }
= { d 1 ⊗ · · · ⊗ d s ⊗ d 0 ∈ P D ( s, 2 m ) |
∃ d i (0 ≤ i ≤ s ) Tr d i = 0 } AG ( s, 2 m ) := π 2 m ( D ( s, 2 m ) ∩ G m ( R 2 m ))
MAS:=maximal antipodal set Theorem 3. (T.-Tasaki)
(1) MAS of G m ( R 2 m ) ∗ is SO (2 m ) ∗ -congruent
to AG ( s, 2 m ) (0 ≤ s ≤ k ) with exceptions ( ∗ ).
(2) MAS of G m ( C 2 m ) ∗ is U (2 m ) ∗ -congruent to AG ( s, 2 m ) ∪ π 2 m ( √
− 1 N D ( s, 2 m )) (0 ≤ s ≤ k ) with exceptions ( ∗ ).
(3) MAS of G m ( H 2 m ) ∗ is Sp (2 m ) ∗ -congruent to AG ( s, 2 m ) ∪ π 2 m ( { i , j , k } N D ( s, 2 m )) (0 ≤ s ≤ k ) with exceptions ( ∗ ).
( ∗ ) : AG ( k − 1 , 2 k ) when 2 m = 2 k and AG (0 , 4) when 2 m = 4.
AG (0 , 4) = π 4 ( {± I 1 ⊗ 1 2 , ± 1 2 ⊗ I 1 , ± I 1 ⊗ I 1 } )
( AG (2 , 4).
6. The 2-number and great antipodal sets of G m ( K 2 m ) ∗
AG C ( s, 2 m ) := AG ( s, 2 m ) ∪ π 2 m ( √
− 1 N D ( s, 2 m )) AG H ( s, 2 m ) := AG ( s, 2 m ) ∪ π 2 m ( { i , j , k } N D ( s, 2 m )) Since N D (0 , 2 m ) = ∅ , AG (0 , 2 m ) = AG C (0 , 2 m )
= AG H (0 , 2 m ).
AG ( s, 2 m ) ( AG C ( s, 2 m ) ( AG H ( s, 2 m )
(1 ≤ s ≤ k )
| AG (0 , 2 m ) | = | π 2 m (∆ m 2 m ) | =
(
2 m m
)/
2
| AG ( s, 2 m ) |
= 2
m
2s−1
− 1
(2 2 s − 1 + 2 s − 1 − 1) +
(
m/ 2
s−1m/ 2
s)/
2
| AG C ( s, 2 m ) |
= 2
m
2s−1
− 1
(2 2 s − 1) +
(
m/ 2
s−1m/ 2
s)/
2
| AG H ( s, 2 m ) |
= 2
m
2s−1
− 1
(2 2 s +1 − 2 s − 1) +
(
m/ 2
s−1m/ 2
s)/
2
(1 ≤ s ≤ k ) We set
(
m/ 2
s−1m/ 2
s)
= 0 when m/ 2 s ∈ / Z . We can show: when m ≥ 5,
| AG (0 , 2 m ) | > | AG H ( s, 2 m ) | > | AG C ( s, 2 m ) | >
| AG ( s, 2 m ) | (1 ≤ s ≤ k ).
We need a case-by-case argument when m ≤ 4.
GAS:=great antipodal set Theorem 4. (T.-Tasaki)
GAS of G m ( K 2 m ) ∗ (up to congruence) and
# 2 G m ( K 2 m ) ∗ are as follows.
I. G m ( R 2 m ) ∗
(1) m = 1 AG (1 , 2) , # 2 G 1 ( R 2 ) ∗ = 2 (2) m = 2 AG (2 , 4) , # 2 G 2 ( R 4 ) ∗ = 9
(3) m = 4 AG (0 , 8) , AG (3 , 8) , # 2 G 4 ( R 8 ) ∗ =
35
(4) m ̸ = 1 , 2 , 4 AG (0 , 2 m ) , # 2 G m ( R 2 m ) ∗ =
(
2 m m
)
/ 2
II. G m ( C 2 m ) ∗
(1) m = 1 AG C (1 , 2) , # 2 G 1 ( C 2 ) ∗ = 3 (2) m = 2 AG C (2 , 4) , # 2 G 2 ( C 4 ) ∗ = 15 (3) m = 3 AG C (1 , 6) , # 2 G 3 ( C 6 ) ∗ = 12 (4) m = 4 AG C (3 , 8) , # 2 G 4 ( C 8 ) ∗ = 63
(5) m ̸ = 1 , 2 , 3 , 4 AG C (0 , 2 m ) , # 2 G m ( C 2 m ) ∗ =
(
2 m m
)
/ 2
III. G m ( H 2 m ) ∗
(1) m = 1 AG H (1 , 2) , # 2 G 1 ( H 2 ) ∗ = 5 (2) m = 2 AG H (2 , 4) , # 2 G 2 ( H 4 ) ∗ = 27 (3) m = 3 AG H (1 , 6) , # 2 G 3 ( H 6 ) ∗ = 20 (4) m = 4 AG H (3 , 8) , # 2 G 4 ( H 8 ) ∗ = 119
(5) m ̸ = 1 , 2 , 3 , 4 AG H (0 , 2 m ) , # 2 G m ( H 2 m ) ∗ =
(
2 m m
)