Acta Mathematica Academiae Paedagogicae Ny´ıregyh´aziensis 31 (2015), 139–151
www.emis.de/journals ISSN 1786-0091
EINSTEIN EQUATIONS OF G-NATURAL COMPLEX FINSLER METRICS
ANNAM ´ARIA SZ ´ASZ
Dedicated to Professor Lajos Tam´assy on the occasion of his 90th birthday
Abstract. In this paper, we endow the holomorphic tangent bundle with a generalized Sasaki type liftGof the fundamental metric tensor of a complex Finsler space. In order to build the Einstein equations on the holomorphic tangent bundle, we determine the Levi-Civita complex linear connection corresponding to this metric. As an application, we give some solutions of the complex Einstein equations in a weakly gravitational space.
1. Preliminaries
In the papers [3, 4] are studied complex Einstein equations for the weakly gravitational field and for complex version of Schwartzschild metric. This study is based on the idea to write the complex Einstein equations for these metrics relative to the Chern-Finsler connection, which is metrical but with torsion. For such theory to be consistent some restrictions are required, called conservation laws, because the connection used is with torsion.
An alternative to this theory is the one expressed in the following. We extend the metric structure of the weakly gravitational field to one on the holomorphic tangent bundle T0M of a complex manifold M, and we then consider the Levi-Civita connection of this lifted metric, which is metrical and torsion-free. Therefore the complex Einstein equations with respect to the Levi-Civita connection have the classical from. In particular, if the space is vacuum the complex Einstein equations reduce to the vanishing of the complex Ricci tensor. Basically, the idea seems to be simple, but the first problem is how to get such a lift and how they can be general. Then is the issue of writing
2010Mathematics Subject Classification. 53B40, 53C60.
Key words and phrases. Holomorphic tangent bundle, Chern-Finsler connection, complex Einstein equations.
This paper is supported by the Sectoral Operational Programme Human Resources De- velopment (SOP HRD), ID134378 financed from the European Social Fund and by the Romanian Government.
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the curvature tensors and Ricci tensors onT0M. For this we turn again to the well-known adapted frames of Chern-Finsler connection, and express all in this complex adapted frames. A similar idea has been applied to the real case by M. Anastasiei and H. Shimada, [5]. Finally, we propose to solve these complex Einstein equations, at least in same particular cases of weakly gravitational metric.
Let M be a complex manifold of complex dimension n. We consider z ∈ M, and so z = (z1, . . . , zn) are complex coordinate in a local chart. Since zk = xk +√
−1xk+n, k = 1, . . . , n, the complex coordinates induce the real coordinates {x1, x2, . . . , x2n} on M. Let TRM be the real tangent bundle. Its complexified tangent bundle TCM splits into the sum of holomorphic tangent bundleT0M and its conjugate T00M, under the action of the natural complex structure J on M. The holomorphic tangent bundle T0M is itself a complex manifold, and the coordinates in a local chart will be denoted by u= (zk, ηa), k, a= 1, . . . , n. withηa =ya+√
−1ya+n, a= 1, . . . , n. Trough this paper the indices i, j, k, . . . and a, b, c, . . . run over {1, . . . , n}, where the second denotes geometric objects in local fibers of the holomorphic tangent bundle. This notation of the indices is important for the clarity of the notions in geometry of T0M manifold.
Consider the sections of the complexified tangent bundleTCM. LetV T0M ⊂ T0(T0M) be the vertical bundle, locally spanned by
n ∂
∂ηa
o
a=1,n, and V T00M its conjugate. The idea of the complex non-linear connection, briefly c.n.c. is an instrument in ‘linearization’ of the geometry of T0M manifold. A c.n.c. is a supplementary subbundle to V T0M in T0(T0M), i.e. T0(T0M) = HT0M ⊕ V T0M. The horizontal distribution HuT0M is locally spanned by
(1) δ
δzk = ∂
∂zk −Nka ∂
∂ηa,
whereNka(z, η) are the coefficients of the c.n.c. The pair{δk:= δzδk, ∂˙a:= ∂η∂a} will be called the adapted frame of the c.n.c., which obey the transformation laws δk = ∂z∂z0kjδ0j and ˙∂a = δakδjb∂z∂z0kj∂˙b0, where δka is the Kronecker symbol. By conjugation everywhere we obtain an adapted frame{δk¯,∂˙¯a}onTu00(T0M). The dual adapted frame are {dzk,dηa} and {d¯zk,d¯ηa} its conjugate, where
(2) δηa = dηa+Nka(z, η)dzk.
Let N be a c.n.c. on T0M. An h−metric onT0M is a d−tensor field hG = gj¯k(z, η)dzj ⊗d¯zk, with gj¯k(z, η) = gk¯j(z, η), detkgj¯k(z, η)k 6= 0. A v−metric onT0M is a d−tensor field vG =ha¯b(z, η)δηa⊗δη¯b, with ha¯b(z, η) =hb¯a(z, η), detkha¯b(z, η)k 6= 0. From here we obtain that an (h, v)−metric on T0M is tensor field G=hG+vG. So, this metric will be written in the next form:
(3) G(z, η) =gjk¯(z, η)dzj⊗d¯zk+ha¯b(z, η)δηa⊗δη¯b.
A distinguished complex linear connection, briefly d-c.l.c., D on T0M is called compatible with the metricG if DG = 0.
Definition 1. An n−dimensional complex Finsler space is a pair (M, F), where F :T0M →R+ is a continuous function satisfying the conditions:
a) L:=F2 is smooth on T]0M :=T0M \ {0};
b) F(z, η)≥0, the equality holds if and only if η= 0;
c) F(z, λη) =|λ|F(z, η) for ∀λ∈C; d) the Hermitian matrix
(4) gj¯k=δajδbk ∂2L
∂ηa∂η¯b, is positive-definite onT]0M.
Then, gj¯k is called the fundamental metric tensor of the complex Finsler space. Consequently, fromc) we have ∂η∂Laηa= ∂¯∂Lηaη¯a=L, ∂g∂ηja¯kηa= ∂g∂¯ηjak¯η¯a = 0, and L=δajδkbgj¯kηaη¯b.
From [1, 7] we know there exists a unique metric Hermitian connection D, of type (1,0)−type, which satisfies in addition DJ XY = J DXY, for all X horizontal vectors, called the Chern-Finsler connection, in brief C-F, which have a special meaning in complex Finsler geometry. The C-F connection DΓ = (Nja, Lijk, Cbca,0,0) is locally given by the following coefficients:
(5) Nja =δkaδblgmk¯ ∂glm¯
∂zj ηb =δkaδblLkljηb; Lhjk =g¯lhδkgj¯l; Cbca =δhaδbjg¯lh∂˙cgj¯l, where the non-vanishing expressions of the C-F connection areDδkδj =Lhjkδh, D∂˙b
∂˙a=Cabd∂˙d and its conjugates.
A particular situation of thed−tensor gjk¯ from (4) is:
Definition 2. Ifgj¯kdepends only on the variablez, then we say that the space (M, F) is purely Hermitian.
The metric tensorgj¯kfrom (4) determines a metric structureGSonTC(T0M), called the Sasaki lift of gjk¯, [7], p.96:
(6) GS =gj¯kdzj ⊗d¯zk+δjaδbkgjk¯(z, η)δηa⊗δη¯b.
We introduce a generalization of the lift (6), which defines also an (h, v)−metric onTC(T0M):
(7) G(z, η) =gjk¯(z, η)dzj⊗d¯zk+ha¯b(z, η)δηa⊗δη¯b,
where gj¯k is the fundamental metric tensor of the Finsler space (M, F), and ha¯b is an arbitraryd−tensor of (0,2)−type.
2. The Levi-Civita connection on T0M
From the standard definition of a complex linear connection on the man- ifold T0M, extended on the complexified tangent bundle TC(T0M), a com- plex linear connection ∇ can be decomposed in the sum ∇ = ∇0 + ∇00, where ∇0: Γ(TC(T0M)) → Γ(TC(T0M)⊗T0(T0∗M)) and ∇00: Γ(TC(T0M)) → Γ(TC(T0M)⊗T00(T0∗M)), which can be decomposed in
∇0 =∇0h+∇0v and∇00 =∇00h+∇00v.
So, in the adapted frame of the C-F c.n.c. {δk,∂˙a, δ¯k,∂˙¯a}, ∇ is defined by the following coefficients:
∇δkδj =
1
Lijkδi+
2
Adjk∂˙d+
3
A¯ıjkδ¯ı+
4
Adjk¯ ∂˙d¯; (8)
∇δk∂˙a =
1
Baki δi+
2
Ldak∂˙i+
3
B¯akı δ¯ı+
4
Bakd¯ ∂˙d¯;
∇δkδ¯j =
1
D¯ijkδi+
2
D¯jkd ∂˙d+
3
L¯ı¯jkδ¯ı+
4
D¯jkd¯∂˙d¯;
∇δk∂˙¯a =
1
E¯aki δi+
2
E¯akd ∂˙d+
3
E¯¯akı δ¯ı+
4
Ldak¯¯ ∂˙d¯;
∇∂˙bδj =
1
Cjbi δi +
2
Fjbd∂˙d+
3
Fjb¯ıδ¯ı+
4
Fjbd¯∂˙d¯;
∇∂˙b
∂˙a =
1
Giabδi+
2
Cabd∂˙d+
3
G¯ıabδ¯ı+
4
Gdab¯∂˙d¯;
∇∂˙bδ¯j =
1
H¯jbi δi +
2
H¯jbd∂˙d+
3
C¯jb¯ı δ¯ı+
4
H¯jbd¯∂˙d¯;
∇∂˙b
∂˙¯a =
1
M¯abi δi+
2
Mab¯d∂˙d+
3
M¯ab¯ı δ¯ı+
4
Cab¯d¯∂˙d¯
and its conjugates, by∇X¯Y¯ =∇XY.
Since ∇G= 0 and ∇ is a symmetric connection, direct calculus leads to Theorem 1. The Hermitian manifold (T0M, GH) admits a unique complex linear connection, which is symmetric and metrical in respect toG, defined by (3). This is called the Levi-Civita connection on T0M, and its local coefficients are represented in the local adapted frame {δk,∂˙a, δk¯,∂˙¯a} by the following non- zero expressions:
1
Lijk = 1
2g¯li(δkgj¯l+δjgk¯l);
2
D¯jkc =−D4ck¯j = 1
2[δ¯jNkc−hdc¯( ˙∂d¯gk¯j)];
(9)
2
Lcak = 1
2[hdc¯(δkhad¯) + ˙∂aNkc];
2
Eakc¯ = 1
2hdc¯[( ˙∂¯aNke)hed¯−( ˙∂d¯Nke)he¯a];
3
Lijk¯ =
1
Dkji¯ = 1
2g¯li(δk¯gj¯l−δ¯lgj¯k);
2
Fjbc = 1
2[hdc¯(δjhad¯)−∂˙aNjc];
4
Lcak¯ =
2
Hka¯c = 1
2hdc¯[δ¯khad¯−( ˙∂d¯Nk¯e¯)ha¯e];
1
Giab = 1
2g¯li[( ˙∂bN¯ld¯)had¯+ ( ˙∂aN¯ld¯)hbd¯];
1
Ckai =
1
Baki = 1
2g¯li[ ˙∂agk¯l+ (δkN¯ld¯)had¯];
4
Hjc¯b =−1
2hdc¯[( ˙∂d¯Nje)he¯b+ ( ˙∂¯bNje)hed¯];
2
Cabc = 1
2hdc¯( ˙∂bhad¯+ ˙∂ahbd¯);
1
M¯abi =
3
Mb¯ia= 1
2g¯li[( ˙∂a¯N¯ld¯)hbd¯−δ¯lhb¯a];
3
Cji¯b =
1
E¯aji = 1
2g¯li[ ˙∂¯bgj¯l−(δ¯lNjd)hd¯b];
4
Cac¯b =
2
M¯bac = 1
2hdc¯( ˙∂¯bhad¯−∂˙d¯ha¯b), and its conjugates.
This connection is not h- or v-metrical.
To study the Levi-Civita connection, we may consider a similar connection, which help us to express easier the different properties of the Levi-Civita con- nection. Indeed let De be a d-c.l.c. on TC(T0M):
Deδkδj =
1
Lijkδi; Deδk∂˙a =
2
Ldak∂˙d; Deδkδ¯j =
3
Li¯jkδ¯ı ; Deδk∂˙a=
4
Ldak∂˙d; (10)
De∂˙aδj =
1
Cjai δi; De∂˙b
∂˙a =
2
Cabd∂˙d; De∂˙aδ¯j =
3
C¯ja¯ı δi ; De∂˙b
∂˙a¯ =
4
C¯abd¯∂˙d and its conjugates, where the local coefficients are expressed in (9).
This d-c.l.c. is metrical with respect to G, i.e.
(11) gj¯k|m =gjk¯|d=gj¯k|m¯ =gjk¯|d¯=ha¯b|m =ha¯b|d =ha¯b|m¯ =ha¯b|d¯= 0, where with ”|”, ”|”, ”¯|”, ”¯|” are notated the h−, v−, ¯h− and ¯v−covariant derivatives with respect to D.e
Proposition 1. The non-zero components of the torsion of the d-c.l.c. De are hTe(δk¯, δj) = eτjik¯δi; vTe(δ¯k, δj) =Θedj¯k∂˙d; hTe( ˙∂¯a, δj) = Υeij¯aδi; hTe( ˙∂a, δj) =Qeijaδi; (12)
vTe( ˙∂¯b,∂˙a) =χeda¯b∂˙d; vTe( ˙∂¯a, δj) = ρedj¯a∂˙d; vTe(δ¯k,∂˙a) = Σeda¯k∂˙d; vTe( ˙∂a, δj) =Pejad∂˙d; and their conjugates.
After a straightforward computation we obtain the expressions for (12) e
τji¯k=
3
Lij¯k; Θedjk¯ =δk¯Njd; Υeij¯a =
3
Cj¯ia; Qeija=
1
Cjai ; (13)
e χda¯b =
4
Cad¯b;ρedj¯a= ˙∂¯aNjd; Σedb¯j =
4
Ldb¯j; Pejad = ˙∂bNjd−L2djb.
The curvature ofDe has twenty components in the form (see p. 44 of [7]):
Reijkh =Ahk{δh
1
Lijk +
1
Lmjk
1
Limh}; (14)
Re¯ı¯jkh =Ahk{δh
3
L¯ı¯jk +
3
Lm¯jk¯
3
L¯ımh¯ };
Reij¯kh =δh
3
Lij¯k−δ¯k 1
Lijh+
3
Lmj¯k 1
Limh−L3im¯k 1
Lmjh+ (δhN¯k¯e)
3
Cj¯ie−(δ¯kNhe)
1
Cjei ; Ωedakh =Ahk{δh
2
Liak +
2
Leak
2
Ldeh}; Ωed¯akh¯ =Ahk{δh
4
Ld¯ak¯ +
4
Le¯ak¯
4
Ldeh¯¯}; Ωeda¯kh =δh
4
Lda¯k−δ¯k 2
Ldah+
4
Lea¯k 2
Ldeh−L4de¯k 2
Leah+ (δhN¯k¯e)
4
Ca¯de−(δ¯kNhe)
2
Caed; Πeijkc = ˙∂c
1
Lijk −δk
1
Cjci +
1
Lmjk
1
Cmci −L1imk
1
Cjci + ( ˙∂cNke)
1
Ceji ; Πe¯¯ıjkc = ˙∂c
3
L¯ı¯jk −δk
3
C¯¯jcı +
3
L¯mjk
3
C¯mcı −L¯3ımk
3
C¯jc¯ı + ( ˙∂cNke)
3
Cei¯j; Πeijkc = ˙∂c
3
Lijk −δk
1
Cjci +
3
Lmjk
1
Cmci −L3imk
1
Cjcm+ ( ˙∂cNke)
1
Cjei ; Peakcd = ˙∂c
2
Ldak −δk
2
Cacd +
2
Leak
2
Cecd −L2dek
2
Cace + ( ˙∂cNke)
2
Caed; Peakcd = ˙∂c
4
Ldak −δk
4
Cacd +
4
Leak
4
Cecd −
4
Ldek
4
Cace + ( ˙∂cNke)
4
Caed; Peakcd = ˙∂c
4
Ldak −δk
2
Cacd +
4
Leak
2
Cecd −L4dek
2
Cace + ( ˙∂cNke)
4
Caed; Θeijbh =δh
3
Cjbi −∂˙b
1
Lijh+
3
Cjbm
1
Limh−C3mbi
1
Lmjh−( ˙∂bNhe)
1
Cjei ; Qedabh =δh
4
Cabd −∂˙b
2
Ldah+
4
Cabe
2
Ldeh−C4ebd
2
Leah−( ˙∂bNhe)
2
Cjed; Ξeijbc =Acb{∂˙c
1
Cjbi +C1jbm
1
Cmci }; Ξe¯ı¯jbc =Acb{∂˙c
3
C¯jb¯ı +
3
C¯jbm¯
3
Cmc¯ı¯ }; Ξeijbc = ˙∂c
3
Cjbi −∂˙b
1
Cjci +
3
Cjbm
1
Cmci −C3mbi
1
Cjcm; Seabcd =Acb{∂˙c
2
Cabd +
2
Cabe
2
Cecd}; Se¯abcd¯ =Acb{∂˙c
4
C¯abd¯ +
4
C¯abe¯
4
C¯ecd¯}; Sead¯bc = ˙∂c
4
Cad¯b−∂˙¯b 2
Cacd +
4
Cae¯b 2
Cecd −C4ed¯b 2
Cace ,
where Ahk means the difference between the terms in the brackets and the terms obtained by replacingk with h.
3. Pure Hermitian metric
The geometrical objects associated withGare generally complicated. Some simplifications appear for particular choices for gjk¯ and ha¯b. We studied in a previous paper, [9], the case δjaδ¯¯kbha¯b = a(F12)gj¯k, and G. Munteanu and N.
Aldea studied the case δajδ¯b¯kha¯b = gj¯k, [7, 2]. Here we resume for a detailed analysis the following particular case of the Sasaki type metric:
(15) GH(z, η) =gj¯k(z)dzj⊗d¯zk+ha¯b(z)δηa⊗δη¯b.
The Chern-Finsler c.l.c. of the complex Finsler space (M, F) is reduced to
CF
DΓ = Nja=δaiδblgmi ∂g¯ ∂zlmj¯ηb, Lijk =gmi ∂g¯ ∂zkjm¯ ,0,0,0
. Thev−and ¯v−covariant derivatives coincides with the partial derivatives with respect to ηa and ¯ηa, respectively. By direct calculation we prove:
Proposition 2. The Levi-Civita connection of the metric (15) is given by the following non-zero coefficients
1
Lijk = 1
2g¯li(∂kgj¯l+∂jgk¯l);
(16)
2
Lcak = 1
2[hdc¯(∂khad¯) + ˙∂aNkc];
3
Lij¯k=
1
Di¯kj = 1
2g¯li(∂k¯gj¯l−∂¯lgj¯k);
4
Lca¯k=
2
H¯kac = 1
2hdc¯[∂¯khad¯−( ˙∂d¯N¯k¯e)ha¯e];
2
Fjbc = 1
2[hdc¯(∂jhad¯)−∂˙aNjc];
1
M¯abi =
3
Mb¯ia= 1
2g¯li[( ˙∂a¯N¯ld¯)hbd¯−∂¯lhb¯a], where ∂k= ∂z∂k.
The curvature of the d-c.l.c.De from (15) is reduced to Reijkh =Ahk{∂h
1
Lijk+
1
Lmjk
1
Limh}; (17)
Re¯ı¯jkh =Ahk{∂h
3
L¯ı¯jk+
3
Lm¯jk¯
3
L¯ımh¯ }; Reij¯kh =∂h
3
Lijk¯−∂¯k 1
Lijh+
3
Lmj¯k 1
Limh−L3im¯k 1
Lmjh; Ωedakh =Ahk{∂h
2
Liak+
2
Leak
2
Ldeh}; Ωed¯akh¯ =Ahk{∂h
4
Ld¯ak¯ +
4
L¯e¯ak
4
Ldeh¯¯ }; Ωeda¯kh =∂h
4
Ldak¯−∂¯k 2
Ldah+
4
Lea¯k 2
Ldeh−L4dek¯ 2
Leah.
Let K be the curvature tensor field of the Levi-Civita connection ∇. We shall denote its components by the same letters as N. Aldea in [2], indexed with two types of indices with the understanding that different indices means