1. Introduction
In every Kähler class of a compact almost homogeneous manifold with two ends, we found some Maxwell–Einstein metrics in [
1].
In every Kähler class of a compact almost homogeneous manifold with two hyper-surface ends we found some
k-generalized Maxwell–Einstein metric defined by Futaki and Ono conformally related to a metric for any
in [
2].
In this paper, we shall prove that for almost homogeneous manifolds with two ends such that one of them is a complex hyper-surface, for any integer , there is always a Kähler metric in the given Kähler class that is related to a Futaki–Ono k generalized Maxwell–Einstein metric.
Definition 1. For any given Kähler class, there is a Maxwell–Einstein metric conformally related to the Kähler class if is an Hermitian metric with a constant scalar curvature such that u is the Hamiltonian function of a holomorphic vector field related to a Kähler metric g in the given Kähler class.
Definition 2. For any given Kähler class, there is a Futaki–Ono k generalized Maxwell–Einstein metric [3,4,5] conformally related to the Kähler class if is an Hermitian metric with a constant scalar curvature such that u is the Hamiltonian function of a holomorphic vector field related to a Kähler metric g in the given Kähler class. Remark 1. This can be found in [5]. LeBrun’s definition [6,7] for a Einstein–Maxwell metric is following: Let be a connected, oriented Riemannian 4-manifold. We will say that h is an Einstein-Maxwell metric if there is a 2-form F on M such that the pair satisfies the Einstein–Maxwell equations and . Here, r is the Ricci curvature of h and the subscript indicates the trace-free part with respect to h. In [6,7], LeBrun proved that Einstein-Maxwell + strongly Hermitian = Maxwell–Einstein. For example, see [7] Proposition 5. The condition of a strongly Hermitian is that (1) the metric is Hermitian, and (2) the curvature is some kind of Kähler-like. This is a far more stronger condition than to be a Riemannian metric. Also, all the Kähler metrics with constant scalar curvatures satisfy the conditions in both Definitions 1 and 2 with u being any positive constant. In these cases, the corresponding holomorphic vector fields are zeros. Even for the real dimension 4, the Maxwell–Einstein metrics are much more than Calabi extremal metrics. Question 1. Is there any compact Einstein-Maxwell metric other than our Maxwell–Einstein metrics?
Our point here is that these two concepts are quite different.
Proposition 1 ([
1])
. For any Kähler class on a compact almost homogeneous manifold with two ends, there is at least one Maxwell–Einstein metrics in the given Kähler class. In [
2], we proved the following:
Proposition 2 ([
2])
. For any Kähler class on a compact almost homogeneous manifold with two hyper-surface ends, there is at least one Futaki–Ono k-generalized Maxwell–Einstein metrics in the given Kähler class for any . In this paper, we are able to prove the following:
Theorem 1. For any Kähler class on a compact almost homogeneous manifold with two ends and one of them being a complex hyper-surface, for any integer , there is at least one Futaki–Ono k generalized Maxwell–Einstein metrics in the given Kähler class.
We notice that when the complex dimension of the manifold M is 2, some Calabi extremal Kähler metrics, e.g., on blow up a point, are actually the same as the Maxwell–Einstein metrics. Moreover, in that case, the corresponding Hermitian metrics are actually Hermitian–Einstein as Riemannian manifolds.
Therefore, Maxwell–Einstein metrics should be as standard as Calabi extremal metrics. But Maxwell–Einstein metrics are not in general Einstein metrics just as quaternion Kähler are not in general Kähler.
Recently, after the publications of a series of LeBrun’s papers, e.g., [
6,
7] and the references therein, it seems to us that Maxwell–Einstein metrics became a hot topic in the mathematical community. In fact, LeBrun has found many Maxwell–Einstein metrics on the Hirzebruch surfaces. That is the special case for our earlier results with the base manifold to be
. We finally published our earlier work in [
1] on this aspect.
There are also many interesting papers on this aspect, for example, [
8,
9,
10,
11,
12,
13]. In [
9], they proved that on any admissible Kähler class, there is an extremal Maxwell–Einstein metric with a given number
. That is, the scalar curvature is a potential function of a holomorphic vector field. This is more like a soliton version of the Maxwell–Einstein metrics. Therefore, their results do not imply our earlier results. Also, the admissible metrics are very restricted and do not include all the compact almost homogeneous Kähler manifolds with two ends.
One also notice that most people called these metrics Einstein–Maxwell. These metrics understandably came from physics. Professor LeBrun worked on these metrics for many years without our notice. Some of them are actually Hermitian–Einstein in the Riemannian sense. But our metrics are generally quite different. To make the difference, we call them Maxwell–Einstein metrics instead. They are more like some kind of pseudo-Einstein metrics as Calabi extremal metrics. Just as the tangent vectors of curves related to the velocities of motions, Riemannian geometry related to general relativity, fiber bundles theory related to Yang-Mills theory, Calabi-Yau threefolds related to supersymmetries, Calabi extremal metrics related to Page’s special Hermitian–Einstein metrics [
14] (see [
15], for example), the Maxwell–Einstein metrics (we found in the late 1900’s and early 2000’s in an effort to combine the Kähler geometry with conformal geometry) might even be a better way to relate Page’s Einstein metrics and the Einstein–Maxwell equations from the physics, for which we unfortunately are not experts in any sense.
In this paper, we basically followed the line of the proof in [
1], or even earlier in [
16], and [
17,
18,
19,
20] (with the last two papers the second author noticed even before he moved to University of California at Berkeley). After a transformation, the related equation becomes an ordinary differential Equation (
12). In [
1], after manipulations, the equation became a simple equation of a second derivative of certain function. One could just solve it by integrating twice. Here, as in [
2], it is a little bit more complicated. Fortunately, we can still integrate once by finding a number
A and a power
s, and transfer the equation into (16). Fortunately and unfortunately,
s has two solutions. Even if in the classical case when
, by (19)
s can be either
or
. In that case, the number
in (18) is either 0 or
. Zero is the classical case but negative two is not. This is interesting.
Fortunately, s and B do not depend on a. After this, we obtained (20), which is a first-order linear equation and can be solved. Also, in (21) and in (22) are smaller than . Most arguments can be carried through.
The existence Lemma (Lemma 8) still work after hard efforts. A complete proof is given in
Section 3. One can even see the duality of the two possible
s in the proof of Lemma 8. The proof is very difficult this time and we turned out receiving heavy help from computers. First, we do a regular proof for
. Then we use the computers for
. The detail calculation with Mathematica for the case with
is given in
Appendix A. Others are similar. This could only be done in nowadays, we guess. Even so, the power of computer could only do finite work this time. We need a complete different method for the infinite possible
k’s. Therefore, in this article, we only do the calculation for
. And we shall leave the rest of the proof of the existence Lemma to the next paper unfortunately. However, for the existence Lemma we can do for all of these manifolds with two ends (hyper-surfaces or not).
The next difficult part in the proof is the proof of the positive Lemma (Lemma 9) in our
Section 4. Our earlier arguments in both [
1,
2] again just do not quite work. Fortunately, we could handle in the cases in which one of the end is a complex hyper-surface. The proof is even harder than the existence in this paper, and is one of core of this paper. Therefore, in this paper the manifold itself is a completion of a line bundle.
We conjecture that the similar result is true for all the compact almost homogeneous Kähler manifold with two ends.
Ref. [
2] is the second chapter of the first author’s dissertation with a page number of 173 in Henan University with
Section 2 (in this paper) as a subsection 1.2.2. This paper is the chapter 3 (our
Section 3) from page 25 to 62, and the chapter 6 (our
Section 4) from page 145 to 164. Therefore, we purposely repeat some parts of this paper from [
2] to make things easier for the readers and the reviewers, e.g., the introduction and
Section 2. Also, our
Section 4 has some of the first part and the last part similar to [
2]. The reason is that the purposes are similar, to prove the positivity. However, our
Section 4.1,
Section 4.2 and
Section 4.3 are completely different. Other parts of our paper, in particular,
Section 4 are also quite different from [
2].
Also, we might keep performing the same computer calculation for bigger k’s. However, first when k is bigger, it requires more computing power for a computer. Eventually, it might not be doable. Second, one can not keep performing this even if we have a computer with a infinite computing power. Therefore, in the chapters 4 and 5, from page 63 to 144, of the dissertation of the first author, we use two complete different methods to finish the proof for (1) and (2) .
The most difficult cases are the proof of the existence for the possible situations in which both ends are not hyper-surface. The difficulty is not the existence of solution, but the positivity of the solution, which we are still working on it.
Remark 2. As mentioned in our Question 1, all the known Einstein–Maxwell metrics (at least in the real dimension 4) are Maxwell–Einstein metrics in the compact case. In [10], they gives an almost Kähler nonKähler Einstein–Maxwell metric on an open four dimensional manifold. However, it seems to us that the original definition of a Einstein–Maxwell metric does not need any almost complex structure, integrable or not. It seems to us the construction actually came from a related Kähler structure. See [10] p. 828, right before “Solution 2:”. Also, the related Lie group is not unimodule from [21] p. 33–34. or . From this fact, we can see the power of the Hermitian methods. Also, there are many explicit examples of Maxwell–Einstein metrics in [7]. Similar Futaki–Ono k-generalized Maxwell–Einstein metrics can be constructed on the Hirzebruch surfaces in the same way according to our result in [2]. 2. Certain Completions of Line Bundles
Our results can be regarded as a continuation of [
1,
2,
16,
18,
19,
20,
22,
23,
24,
25,
26]. We state without detailed proof in this section the Lemmas similar to those in these papers as follows. The readers might take [
16,
23] as the references. Most Lemmas can be actually found in [
16].
Let be a holomorphic line bundle over a compact complex Kähler manifold M and h an Hermitian metric of L. Denote by the open subset 0-section} of L and let be defined by , where is the norm defined by h. Now, we consider function which is only depending on s and is monotone-increasing with respect to s.
Let
be the complex structure of
L and
J be the complex structure of
M. Now, we consider a Riemannian metric on
of the form
where
with
,
is a one parameter family of Riemannian metrics on
M. This form of the metrics is general by using the function
as the length of the geodesics perpendicular to the generic orbits. Define a function
u on
depending only on
by
, where
H be the real vector field on
corresponding to the
action on
.
Lemma 1 (Cf [
19,
20], ([
16] p. 2257))
. Suppose that the range of τ contains 0. Then is Kähler if and only if is Kähler and , where B is the curvature of L with respect to h, .
Throughout this paper, we assume that
- (1)
is a compactification of and is the restriction of a Kähler metric of to .
- (2)
The range of contains 0.
- (3)
The eigenvalues of B with respect to are constants on M.
- (4)
The traces of the Ricci curvature r of g on each eigenvector space of B are constant.
The condition (4) here is much more general than that in [
1,
16] in which we have the following:
- (4)’
The eigenvalues of r are constants.
Our results cover some results which appeared in recent years. For example, if g has a constant scalar curvature and B has only one eigenvalue.
By abusing the language, we call the constants in (4) the trace eigenvalues.
Let be a system of holomorphic local coordinates on M. . Using a trivialization of , we take a system of holomorphic local coordinates on such that .
Here, we notice that
is corresponding to
in [
23] p. 552.
s can be regarded as Re
near the considered point. So
s is the
in [
23] p. 552. As in [
16] we let
as a function of
U and we let
F be the Kähler potential as in [
23] p. 552, then by comparing [
16] Lemma 2 (or the Lemma 4 below) with [
23] p. 552 we immediately have the following:
Lemma 2 (Cf [
23,
24])
. . From
, we obtain
.
is
up to a constant in [
23] p. 552, i.e.,
Lemma 3 (Cf [
23,
24])
. U is the Legendre transformation of s. Here, we use the Legendre transformation in [
23] (or later in [
24], in which we proposed to use the uniform stability and Kähler–Einstein metrics with conic singularity along a divisor to approach the Kähler-Einstein problem) instead of the moment map in [
16] since we need the new insight in the related papers.
Let be the partial differentiations on and be the partial differentiations on M.
Lemma 4 (Cf [
19,
20], Lemma 2 in [
16])
. We havewhere . At the point considered, we can choose a local coordinate system around such that at P, so at the point we considering (see [27], for example), then if f is a function on depending only on τ, we haveThe Ricci curvature at this point iswhere . In particular, we have the scalar curvaturewhere as a function of U and . We also have , . Lemma 5 (Cf. [
28,
29], Lemma 3 in [
16])
. We can also regard U as a moment map corresponding to and just be the symplectic reduction in at . is extremal if and only if for some . Let and , they are complex sub-manifolds, since they are components of the fixed point set of which is semisimple. Let be the codimension of in , be the codimension of in .
Lemma 6 (Cf. Lemma 4 in [
16])
. Suppose that there is another Kähler metrics on in the same Kähler class which is of form on . Letbe the corresponding metric and the corresponding functions of s. Then there is a unique corresponding such that . In this case, (or and , hold. So we may write and . Thenwhere (or is a polynomial of U such that (or and Proof. Let
, then
for
, so at
(or
, therefore there is a
such that
. By choosing
such that
, one sees that
as desired.
The last statement follows from the fact that the scalar curvature R is finite on both and . □
We need normalization in this paper. By rescaling, we can choose for any and , allowing us to assume that and , then .
3. Existence of the Futaki–Ono’s Generalized Maxwell–Einstein Metrics—Existence
We recall our definition of the Futaki–Ono’s Generalized k Maxwell–Einstein metrics: For any given Kähler class, there is a Futaki–Ono’s Generalized k Maxwell–Einstein metric conformally related to the Kähler class if is an Hermitian metric with a constant scalar curvature such that u is the Hamiltonian function of a holomorphic vector field related to a Kähler metric g in the given Kähler class. Also, our n here is the complex dimension of L in last section. Therefore, .
From Lemma 5, it can be seen that if is a Futaki–Ono’s Generalized k Maxwell–Einstein metric, then for some .
From [
30], p. 126, (1), we have
Here,
for the scalar curvature of our Kähler metric in Lemma 4. Notice that here we have a different sign for the Laplacian from [
5].
Remark 3. The notation is directly taken from [5] page 94, Formula (2). Our n here is the m in the Formula (1) there. Therefore, their n was the twice of our n, and is in this paper. From [
2], we then have the following:
where
we need to find an
a in
satisfying the following identity:
where
When , a similar result holds.
Let
with
, Where
l is an integer and
p is not necessarily an integer. Then
Now,
with
, which is equivalent to
when
a turns to 1.
with
, which is equivalent to
when
a turns to 1.
with
, which is equivalent to
when
a turns to 1.
with
, which is equivalent to
when
a turns to 1.
Now, we use the mathematical induction for
l, assuming that when
,
with
, which is equivalent to
when
a turns to 1,
with
, which is equivalent to
when
a turns to 1.
Therefore, by our induction formula we can prove that
is equivalent to
when
a turns to 1.
Here, for the convenience of writing, let
where
l is an integer and
p is not necessarily an integer.
The major part of the difference in the two sides of Equation (
10) comes from
By the formula of
near
in (7) of Lemma 6, we only need to check that
has a negative major part. By (13) it is proportional to the following:
It is determined by the sign of
Simplify (15) below
it is determined by the sign
Simplify (16) below if
This is also true if
. We just do not take out any factor. If
, we multiply some linear factors instead and we obtain the following:
Therefore, it is determined by the sign
We now divide the second term of the above equation by both sides at the same time, we obtain the following:
Taking the log of the first term above expression, we obtain the following:
Taking the derivative of
, we obtain the following:
from (11)
so (19) is a monotonically increasing function of
. Now, we just need to see if (19) is positive or negative when
, when
, (19) becomes
let
then
Therefore, after replacing
i in (20) by
, (20) becomes
If
, it is determined by the sign
because
then
it is determined by the sign
for convenience, we shall use
(or
in the Mathematica calculation) to represent expression (24) below. And our goal is to prove the following:
Claim: .
In this paper, we only deal with the cases in which .
3.1.
If
, then
The expression is as follows
This an odd function. The coefficient of the
term is 2. The constant term and the
terms are zeros. We only need to calculate the coefficient of the
t term. We take the derivative to
t, then let
, we obtain the following:
We obtain the following
when
then
Therefore, we have that the inequality in the Claim holds for . That is, we can find a solution a in the Formula (10).
Theorem 2. A solution a exists for .
3.2.
Using Collect[Expand[fun1[n, 4, t]], t] in mathematica, then
substituting
into
, we obtain
See
Appendix A for a detail of Mathematica calculations.
When
since the
and
terms controls the
term by
, then
Therefore, we have that the inequality in the Claim holds for . That is, we can find a solution a in the Formula (10).
Theorem 3. A solution a exists for .
Using Collect[Expand[fun1[n, 5, t]], t] in mathematica, then
substituting
into
, we obtain
when
since the
term controls the
and
terms by
; 2 term controls the 1 term by
, then
Therefore, we have
Theorem 4. A solution a exists for .
Using Collect[Expand[fun1[n, 6, t]], t] in mathematica, then
substituting
into
, we obtain
when
since the
term controls the
and
terms by
; 4 term controls the 3 term; 2 term controls the 1 term, then
Therefore, we have
Theorem 5. A solution a exists for .
3.3.
Using Collect[Expand[fun1[n, 7, t]], t] in mathematica, then
substituting
into
, we obtain
Here, are two ways we can prove
: when
Lemma 7. If , and x is a positive integer greater than 1, then .
Proof. Differentiating with respect to x yields . Since , it follows that is monotonically increasing. Moreover, when , we have . Therefore, when x is a positive integer greater than 1, we have . □
Now, we want to take the
term and a part of the
term to control the
term. By
and
, we take out
from the
term. We still have more than
left. Now,
and 6 term provide at least
. Again,
. Taking
from 4 term we control the 5 term. The left 4 term controls the 3 term; 2 term controls the 1 term, then
: We can also substitute
into
. We notice that
m is just the complex dimension of the base manifold
M. We obtain the following:
since
then
Therefore, we have
Theorem 6. A solution a exists for .
3.4.
Using Collect[Expand[fun1[n, 8, t]], t] in mathematica, then
substituting
into
, we obtain
substituting
into
, we obtain the following:
since
then
Therefore, we have
Theorem 7. A solution a exists for .
Using Collect[Expand[fun1[n, 9, t]], t] in mathematica, then
substituting
into
, we obtain
substituting
into
, we obtain the following:
since
then
Therefore, we have
Theorem 8. A solution a exists for .
Using Collect[Expand[fun1[n, 10, t]], t] in mathematica, then
substituting
into
, we obtain
substituting
into
, we obtain the following:
since
then
Therefore, we have
Theorem 9. A solution a exists for .
Using Collect[Expand[fun1[n, 11, t]], t] in mathematica, then
substituting
into
, we obtain the following:
substituting
into
, we obtain the following:
since
then
Therefore, we have
Theorem 10. A solution a exists for .
Using Collect[Expand[fun1[n, 12, t]], t] in mathematica, then
substituting
into
, we obtain the following:
substituting
into
, we obtain the following:
since
then
Therefore, we have
Theorem 11. A solution a exists for .
Using Collect[Expand[fun1[n, 13, t]], t] in mathematica, then
substituting
into
, we obtain the following:
substituting
into
, we obtain the following:
since
then
Therefore, we have the following:
Theorem 12. A solution a exists for .
Actually, we already calculated with computer that have all negative coefficients for also. Therefore, these Theorems are also true for . However, it is too long to present them here. Obviously, one can not do these forever. And, we need a new method. We shall finish the proof for the rest in the next paper. For this paper, we just stop here.
However, we can figure out a conjecture:
Conjecture 1. The coefficients of the m terms in are all negative for any integer .
We then have the following:
Lemma 8. There is a solution a for Equation (10) with an integer k if . 4. Existence of the Futaki–Ono’s Generalized Maxwell–Einstein Metrics—Positivity
Let
then
.
Theorem 13 (Cf. [
19], ([
16] Lemma 6))
. There is a generalized Maxwell–Einstein metric in the same Kähler class of if is positive on . Conjecture 2 (Cf. [
1,
16,
31])
. If r has nonnegative trace eigenvalues, then for a given a, Φ
as above is always positive on . In this section, we shall prove this conjecture for the cases in which one of and is 1. That is, our Theorem 14 later on. Therefore, it is true for a completion of a line bundle.
Combining with Lemma 8 in last section, we obtain the existence of the Futaki–Ono k-generalized Maxwell–Einstein metric with any integer for the completion of our line bundles. That is, Theorem 1.
Since the derivative of
is
, we have the following
Diagonalizing
B, we see that
Q is a product of polynomials of degree 1. Let
for convenience, we let
then
denote the distinct roots of
Q for which some corresponding Ricci curvature
is nonzero, where
are positive and
can also be negative,
. On account of
Let
then
Recall that
,
. let
, then
then
Let us consider the case in which only at most three of
are nonzero. Different from the earlier paper [
2], we need to make (7) hold. In our case, both
. That is,
one need
Therefore, if and only is nonzero, we can only have . And, if and only is nonzero, we can only have . If and only is nonzero for those i with , we can only require that one of , for some j with , and one of , for some k with .
That is different from [
2], so we need one of
and equal
if
for an
i with
; and one of
and equal
if
for an
i with
.
So, we need consider several situations: (1) three and two of them with and ; (2) two of them and only one with , the other , ; (3) two of them and only one with , the other , ; (4) two of them and one with , the other ; (5) only one with , and ; (6) only one with , and .
A. We can treat (1) and (4) as one situation. Somehow, (1) is difficult although (4) can be treated. Therefore, we might leave this situation out in this paper and shall try to treat it in the future.
B. (2) and (5) as one; (3) and (6) as one. Also, (2) and (3) are similar. Therefore, we only need to deal with (2) in which we replace by . In these cases, only one of 1 and might be achieved by one of . Therefore, the manifold can be regarded as a completion of a line bundle. On the other hand, all the manifolds which is in a form of a completion of a line bundle are in these cases. Therefore, we only treat these situation in this section.
Therefore, to prove the Conjecture 2 for our cases, we need to prove the following Lemma first:
Lemma 9 (Cf. [
1,
16,
31])
. If r has nonnegative trace eigenvalues and (1) there is only one nonzero , say for example, other than those with or , and (2) either or with or , respectively, then for a given a, Φ
as above is always positive on . Here, we let . Proof of Lemma 9. Let
then
where
We also have when if ; and when if
When
,
on
, and
then
.
4.1. Special Cases
Next, we shall treat our two special cases with either
or
. In the cases in which
and
, for convenience, we replace
U with
y, we need some Lemmas. In this case, the second term in the right side of (29) is zero and we might just replace
by 1. Here, we only assume that
. Otherwise, we just exchange the ends. Therefore, this is the case in which the manifold is a completion of a line bundle over the end at the infinity. Let
here
.
And
, where
Let
We notice that the last term is nonnegative if
.
We also let
We want to prove that the degree three polynomial
only has one zero in
.
We notice that
has two terms:
with a derivative:
which has a zero
other than
;
with a derivative
which has a zero
other than
.
Lemma 10. has a N shape if and . Moreover, is a locally minimal point if and is a locally maximal point . If , is positive on . Otherwise, for but small enough. has a S shape if i.e.,it is always increasing.
Proof. if . That is, . This is always true. □
Similarly, if
then
That is,
We have
. This implies that
. We notice that the right side is smaller than
. Therefore, this could be achieved whenever
is big enough.
We see that
when
. Actually,
also has a zero , and also has a zero . when .
Now, we first consider the case in which
and are ready to obtain some property for
:
Notice that
have a
N shape, we see that
but
Therefore, there is a local maximal point in
which is
.
We also have Therefore, there is a zero point in . Also, Therefore, there is a zero of the derivative in , which must be a local minimal point.
Therefore, we obtain the following:
Lemma 11. has a N shape and has a negative locally maximal point in if and . Moreover, in this case, it has a negative locally minimal point in and has a zero point . In particular, is the only zero of and .
The first term in the second bracket is linear and increasing. The second term is also increasing on
. This gives another proof for Lemma 11.
4.2. The Cases When and
If
,
, then we let
4.2.1. If
If
, then
let
thus,
has no zero point on
.
Lemma 12. If and , has no zero point on .
4.2.2. If
If
,
, then
let
because
is positive on
. Also
thus,
has no zero point on
.
In general, if
,
, then
It is if . Therefore, we only need to deal with .
Then
,
the zero point
of the first term of
is
and the double zero point 1,
if and only if
That is, when
,
. The first term is also positive. We only need to deal with
it has zero points
and
when
,
,
, if and only if
If
, then
. This is always true since the right side is negative.
If
, then
. In this case, we have the following:
. We have the following:
.
Therefore, if
, and
then
,
. This implies
. That is,
. But
. So,
. A contradiction. This implies that
. The function only has one zero.
Therefore, we only need to deal with the case in which . In this case, we still get . Therefore, . That is, . Again, a contradiction. We obtain . It only has one zero. The proof is complete.
Lemma 13. If and , has only one zero point on .
4.3. The Cases in Which and
If
,
, then we let
4.3.1. If
If
, then
let
if
then
,
has no zero point on
; if
then
,
has one zero point on
; thus,
has at most one zero point on
.
Lemma 14. If and , has only one zero point on .
4.3.2. If
If
,
, then
let
then
Let us take the derivative of
over
U, and we will obtain
because of
is monotonically increasing on
.
so
is monotonically increasing on
and because
it implies that
has at most one zero point on
.
In general, if
,
, then
let
and
If
, the second term is positive. By
is increasing, it can only have at most one zero. Therefore, we only need to deal with
.
Then
,
The zero point of the first term of is and the double zero point .
We notice that this is exactly . Applying Lemma 11, we see that it has at most one zero in .
Lemma 15. If and , has only one zero point on .
4.4. Final Proof of the Existence Theorem for the Completion of a Line Bundle
And we shall obtain following our first positive Theorem after our final efforts to the proof of our Lemma 9:
Theorem 14. If our manifold only has one end contracted, that is, the manifold is a completion of a line bundle, the solution we obtained in our earlier Theorems has a positive φ on .
Proof of Lemma 9 (Continue) . Recall that
And
then, from Formula (29)
4.4.1. , , and and Only Another Are Nonzero with
Let us first consider the case in which , , and and only another are nonzero with .
, then
Lemmas 12 and 13 say that has at most one zero on .
If
is not all greater than zero on
, then
has at least one zero. If it has least two zeros, we set them to be
and
let
, then
. There are at least three critical points between them. Let
.
and
near
;
and
nearby;
and
nearby;
and
nearby. Then,
at some point
in
,
at some point
in
and
at some point
in
. That is,
at some point
in
,
at some point
in
and
at some point
in
. But
at 1. That is, there are at least three zeros
,
and
in
. And
has at least two zeros in
, which is a contradiction to our Lemmas 12 and 13.
Similarly, if it has only one zero, we set it to be
, then,
. Then,
is a critical point and there are at least two more critical points between them. Let
with
.
and
near
;
for
and small; also
and
nearby. Then,
at some point
in
,
at some point
in
and
at some point
in
. But
at 1. That is, again, there are at least three zeros
,
and
in
, which is again a contradiction.
Therefore, in the case in our Lemma 9 with , as above is always positive on .
4.4.2. , , and and Only Another Are Nonzero with
Let us second consider the case in which , , and and only another are nonzero with .
, then
Lemmas 14 and 15 say that has at most one zero on .
If
is not all greater than zero on
, then,
has at least one zero. If it has least two zeros, we set them to be
and
let
, then,
. There are at least three critical points between them. Let
.
and
near
;
and
nearby;
and
nearby;
and
nearby. Then,
at some point
in
,
at some point
in
and
at some point
in
. That is,
at some point
in
,
at some point
in
and
at some point
in
. But
at
. That is, again, there are at least three zeros
,
and
in
, which is again a contradiction to our Lemmas 14 and 15.
Similarly, if it has only one zero, we set it to be
, then,
. Then,
is a critical point and there are at least two more critical points between them. Let
with
.
and
near
;
for
and small; also
and
nearby. Then,
at some point
in
,
at some point
in
and
at some point
in
. But
at
. That is, again, there are at least three zeros
,
and
in
, a contradiction.
We proved our Lemma 9 as desired. □
4.4.3. Proof of Theorem 14 (Continue)
Now, let us consider the case of multiple nonzero . First, we need to deal with the case in which all except when (or ) when (resp. ). In this case, we have Lemmas 12 and 14, The arguments in the proof of the Lemma 9 still go through.
Now, we consider the case in which there is at least one nonzero
other than the ones with
(resp.
). Similar to the Lemma 13, let
or in the
case. We want to replace
by
and get a solution with the same numbers
c and
a.
First, we want to determine the number
. We have that
then
and
Then, the corresponding solutions have the property as in our Lemma 9.
In general, we want to find a solution such that
, where
are positive numbers for
. Because
and
then
then
That is,
therefore
as above is always positive on
.
This, in particular, concludes our Theorem 14. □
Now, combining Lemma 8 and Theorem 14, we obtain our Theorem 1.