In this paper, we discuss the uniqueness and existence of local solutions for the perturbed static, spherically symmetric Einstein-Yang-Mills (EYM) equations with gauge group SU(2). Moreover, we show that the rational expression solutions to the equations only happened in traditional Schwarzschild solutions and Reissner-Nordstrom solutions. From these results, we can infer that there is no rational ghost soliton solution for the EYM equations.
Citation: Wenjing Song, Haiyun Deng, Ganshan Yang. Two-uniqueness of rational ghost soliton solution and well-posedness of perturbed Einstein-Yang-Mills equations[J]. AIMS Mathematics, 2021, 6(11): 12065-12076. doi: 10.3934/math.2021699
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In this paper, we discuss the uniqueness and existence of local solutions for the perturbed static, spherically symmetric Einstein-Yang-Mills (EYM) equations with gauge group SU(2). Moreover, we show that the rational expression solutions to the equations only happened in traditional Schwarzschild solutions and Reissner-Nordstrom solutions. From these results, we can infer that there is no rational ghost soliton solution for the EYM equations.
We recall that for the spherically symmetric EYM equations, the Einstein metric is of the form
ds2=−AC2dt2+A−1dr2+r2(dθ2+sin2θdϕ2), | (1.1) |
and the SU(2) Yang-Mills curvature 2-form is
F=w′τ1dr∧dθ+w′τ2∧(sinθdϕ)−(1−w2)τ3dθ∧(sinθdϕ). | (1.2) |
Here A,C and w are functions of r, and (τ1,τ2,τ3) form a basis for the Lie algebra SU(2). Using (1.1) and (1.2), the spherically symmetric SU(2) EYM equations are
rA′+(1+2w′2)A=1−(1−w2)2r2, | (1.3) |
r2Aw″+[r(1−A)−(1−w2)2r]w′+w(1−w2)=0, | (1.4) |
and
C′C=2w′2r. | (1.5) |
We should point out that (1.3) and (1.4) do not involve C.
Neither the vacuum Einstein equations nor the pure Yang-Mills equations have nontrivial static globally regular solutions, so it is natural to conjecture that the coupled EYM equations also have no nontrivial globally regular solutions. In 1988, Bartnik and McKinnon [1] presented numerical evidence for the existence of a discrete family of globally regular solutions of the static EYM equations: the gravitational attraction can balance the Yang-Mills (YM) repulsive force. This prompts the mathematical theory of this conjecture came into being. However, until now, the behavior of the solution in the case of spherical symmetry is still unclear. For example, in 2018, Baxter [2] considered the case of spherical symmetry.
We note that Gross-Pitaevskii equation has been successfully used to deal with Bose-Einstein condensation equation by applying Hirota's method, Lie algebra structure and Backlund transformations, bilinear transform, etc (refer to [3,4,5] and their references), but we have not seen an example of applying these methods to Einstein-Yang-Mills equation.
In this paper, we mainly prove the following surprising properties of static spherically symmetric solutions of the SU(2) Einstein-Yang-Mills equations.
Theorem 1.1. There are no any rational expression solutions for static spherically symmetric solutions to the perturbed SU(2) Einstein-Yang-Mills equations
rA′+(1+2w′2)A=1−(1−w2)2r2, | (1.6) |
r2Aw″+[r(1−A)−(1−w2)2r]w′+λw(1−w2)=0, | (1.7) |
except classical Schwarzschild solutions and Reissner-Nordstrom solutions. Here we add a perturbed coefficient into (1.2), and we assume that λ is waving near 1.
In 1993, Smoller, Wasserman and Yau proved the existence of black hole solutions for the Einstein-Yang-Mills equations (see [7,8,9]). In 1995, Smoller and Wasserman [6] provided a rigorous proof of the existence and uniqueness of the solutions to the Einstein-Yang-Mills equations with gauge group SU(2). After adding the perturbed term λ to (1.4), we discover that the perturbed equations have the same properties as the original equations in existence and uniqueness, see [9].
Theorem 1.2. Let ˉr>0 be given. Assume that A(ˉr)=0, and (ˉw,β) satisfies
Φ(ˉr)β+ˉw(1−ˉw2)=0, |
where Φ(ˉr)=ˉr−(1−ˉw2)2ˉr≠0. Then there exists a unique C2,α solution (A(r,ˉw),w(r,ˉw),w′(r,ˉw)) of (1.6), (1.7) with the initial conditions (A(ˉr,ˉw),w(ˉr,ˉw),w′(ˉr,ˉw))=(0,ˉw,β), defined on some interval ˉr<r<ˉr+s(ˉw). The solution is analytic on |r−ˉr|<s(ˉw), and the one-parameter family (A(r,ˉw),w(r,ˉw),w′(r,ˉw)) is continuous about r and ˉw.
Theorem 1.3. There are no any rational analytic solutions for EYM equations except classical Schwarzschild solutions or Reissner-Nordstrom solutions.
In this section, we prove Theorem 1.1. Set
A=anrn+an−1rn−1+⋯+a1r+a0bmrm+bm−1rm−1+⋯+b1r+b0, | (2.1) |
w=csrs+cs−1rs−1+⋯+c1r+c0dtrt+dt−1rt−1+⋯+d1r+d0, | (2.2) |
where ai, bi, ci, di (i∈[1,n],n≥1) are constants.
To obtain a simple form, we suppose
A=qp, | (2.3) |
w=kh, | (2.4) |
where p,q,h,k represent the corresponding polynomial of denominator and numerator. A and w are simplified, i.e., q,p,h and k are irreducible. Without loss of generality, assuming λ∈(0.5,2) and λ≠1, then (1.6) and (1.7) can be simplified as
h4r3(q′p−p′q)+ph4r2q+2pqr2(k′h−h′k)2=p2h4r2−p2(h2−k2)2, | (2.5) |
r3h2q(k″h3−h″kh2−2k′h2h′+2hkh′2)+(k′h−kh′)[pr2h4−qr2h4−p(h2−k2)2]=λprkh3(k2−h2). | (2.6) |
In the remainder of this paper, we use ˜p, ˜q, ˜h, ˜k to donate the corresponding highest degree of p, q, h, k. Using L1=h4r3(q′p−p′q), L2=ph4r2q, L3=2pqr2(k′h−h′k)2, R1=p2h4r2, R2=−p2(h2−k2)2 to facilitate the writing of (2.5), and using ~L1, ~L2, ~L3, ~R1, ~R2 to donate the corresponding highest degree of L1, L2, L3, R1, R2. Similarly, using L21=r3h2q(k″h3−h″kh2−2k′h2h′+2hkh′2), L22=(k′h−kh′)[pr2h4−qr2h4−p(h2−k2)2], R21=λprkh3(k2−h2) to facilitate the writing of (2.6), and using ~L21, ~L22, ~R21 to donate the corresponding highest degree of L21, L22, R21.
Lemma 2.1. If the solution of the perturbed EYM equations can be written as (2.1) and (2.2). Then
˜p=˜q,˜h≥˜k | (2.7) |
or
˜p<˜q,˜h<˜k | (2.8) |
holds. Moreover, if (2.7) holds, then an=bm. If (2.8) holds, then anbm<0, ˜q−˜p=2(˜k−˜h)≥2. Here A is the form of (2.1).
Proof. It is obvious that p and h can not be zero. To prove this lemma, we start with the simple case and move on to the general case.
When q = 0, i.e., A≡0, then, from (1.6) and (1.7), w≡0, r=1 or w2≡1, r=0.
When k=0, i.e., w≡0, the solution is Reissner-Nordstrom Solution.
When q and p are constants, i.e., A is a constant, this case are included in the later discussion, where we discuss the situation that ˜p=˜q, i.e., p=q, then A≡1 and w2≡1.
When h and k are constants, i.e., w is a constant, then w2≡1 from (1.6) and (1.7), which is corresponding to Schwarzschild Solution.
Next, we discuss the case k≠0, q≠0, and A, w may not be constants. Before observing the highest degree of (2.5) and (2.6) to each terms, we pick out some special cases as which have been discussed above: If q′p−p′q≡0, then A′≡0; If k′h−h′k≡0, then w′≡0; If h2=k2, then w2≡1. Then in the following discussion, each terms in (2.5) can not be constant except R2. Noted that
L1:4˜h+˜p+˜q+2∼4˜h+3; L2:4˜h+˜p+˜q+2;L3:2˜h+2˜k+˜p+˜q∼˜p+˜q+2; R1:4˜h+2˜p+2; R2:max(4˜h,˜k)+2˜p∼2˜p, |
where the part on the right of colon means the highest degree.
Hint: If ˜p=˜q, then ~L1 < 4˜h+˜p+˜q+2. If ˜p≠˜q, then ~L1 = 4˜h+˜p+˜q+2. If ˜h=˜k, then ~L3 < 2˜h+2˜k+˜p+˜q. If ˜h≠˜k, then ~L3 = 2˜h+2˜k+˜p+˜q and ~R2 = max(4˜h, ˜k)+2˜p.
When ˜p=˜q, ˜h<˜k, then ~R2 > max(~L1, ~L2, ~L3, ~R1), which leads to a contradiction; When ˜p=˜q, ˜h≥˜k, then ~L2 = ~R1 > max(~L1, ~L3, ~R2) and an=bn, i.e., A=1, as r→∞.
When ˜p≠˜q, ˜h=˜k, then ~L3≤4˜h+˜p+˜q−2<~L1 = ~L2 = 4˜h+˜p+˜q+2, ~R2≤4˜h+2˜p<~R1 = 4˜h+2˜p+2. If ˜p>˜q, then ~R1 > max(~L1, ~L2, ~L3, ~R2), which leads to a contradiction. If ˜p<˜q, A and w as (2.1) and (2.2), here n−m>0 (an≠0, bm≠0, cs≠0, dt≠0), then the coefficient of highest degree in (L1+L2) is
d4tanbm(n−m+1)≠0, |
hence ~L1+L2=~R1 and ˜q=˜p, which leads to a contradiction.
When ˜p≠˜q and ˜h≠˜k, we have ~L1=4˜h+˜p+˜q+2,~L2=4˜h+˜p+˜q+2,~L3=2˜h+2˜k+˜p+˜q,~R1=4˜h+2˜p+2,~R2=4max(˜h,˜k)+2˜p.
When ˜k>˜h, ˜p>˜q, then ~R2 > max(~L1, ~L2, ~L3, ~R1), which leads to a contradiction.
When ˜k<˜h, ˜p>˜q, then ~R1 > max(~L1, ~L2, ~L3, ~R2), which leads to a contradiction.
When ˜k<˜h, ˜p<˜q, then ~L3 < ~L1 = ~L2 = ~L1+~L2 = 4˜h+˜p+˜q+2 and ~L1+~L2 > ~R1 = 4˜h+2˜p+2 > ~R2. It means that the highest degree of (L1+L2) can not be 4˜h+˜p+˜q+2 from (2.1) and (2.2), here n>m. Calculating the coefficient of highest degree term in L1 and L2, one gets n−m=−1, which leads to a contradiction.
When ˜k>˜h, ˜p<˜q, we consider ˜k=˜h+1 firstly. In this case, we have ~L1=~L2=~L3=4˜h+˜p+˜q+2, ~R2=4˜h+2˜p+4>~R1. Letting
A=anrn+an−1rn−1+⋯+a1r+a0bmrm+bm−1rm−1+⋯+b1r+b0, |
w=ct+1rt+1+ctrt+⋯+c1r+c0dtrt+dt−1rt−1+⋯+d1r+d0, |
and calculating the coefficient of highest degree term in left, one sees that the result of coefficient can not be 0, i.e., ~L1=~L2=~L3=~R2, thus ˜q−˜p=2. Solving the both sides of coefficient of highest degree term, one gets anbm<0. Next, if ˜k>˜h+1, one has ~L3 = 2˜h+2˜k+˜p+˜q = ~R2 = 4˜k+2˜p, hence ˜q−˜p=2(˜k−˜h)>2. What's more, since R2<0, the coefficient of highest degree term to pq in L2 and L3 should be negative, i.e., anbm<0.
Thus Lemma 2.1 holds.
Lemma 2.2. If ˜k>˜h, ˜p<˜q, then ˜k=˜h+1, ˜q=˜p+2.
Proof. In order to prove this lemma, we observe (2.6). Firstly, we consider some simple cases.
When ˜h=0, ˜k=1 and w=ar+b, a≠0, by using coefficient of variation method to (1.6), one can see the expression of A as follows.
If a2≠12, then
A=1+4ab−2a2(b2−1)2a2+1−a42a2+3r2−4a3b2a2+2r−4ab(b2−1)2a2r−(b2−1)2(2a2−1)r2+cr2a2+1, |
where c is a constant. Then we generate the results into (1.7) and discover the fact that
(a52a2+3−a5−λa3)r3+(4a4b2a2+2−4a4b−3λa2b)r2+a(2a2b2−4ab2a2+1−4ab−2a2b2+2a2+λ−3λb2)r+a[(b2−1)22a2−1−(b2−1)2]r−1−acr2a2+λ(4a2−1)(b−b3)=0. For (a52a2+3−a5−λa3)=0 has solutions, one has λ≤2−√3 or λ≥2+√3, which leads to a contradiction.
If a2=12, then
A=2+4ab−b22−116r2−23abr−4ab(b2−1)r−(b2−1)2lnrr2+cr2, |
where c is a constant. Then we generate the results into (1.7) and discover the fact that −a(3+8λ)16r3−b(4+9λ)6r2+[(−12−3λ)ab2−3b+(1+λ)a]r+a(b2−1)2(lnr−1)r−1−acr+λ(b−b3)=0. Let the coefficient of r3 be 0, one gets λ=−38, which leads to a contradiction.
When ˜h=0, ˜k≥2, then ~L21=˜k+˜q+1, ~L22=5˜k+˜p−1, ~R21=3˜k+˜p+1. Through a comparative analysis, one sees ~L22 > max(~L21, ~R21), which leads to a contradiction.
When ˜h=1, then ~L21 ≤ 6+˜k+˜q. If ˜q−˜p≥4, i.e., ˜k−˜h≥2, then ~L22 = 5˜k+˜p, ~R21 = 3˜k+˜p+4. Through a comparative analysis, one gets ~L22 > max(~L21, ~R21), which leads to a contradiction.
When ˜h≥2, if ˜q−˜p≥4, i.e., ˜k−˜h≥2, then ~L21 ≤ 5˜h+1+˜k+˜q, ~L22 = 5˜k+˜h+˜p−1, ~R21 = 3˜k+3˜h+˜p+1. By analysis, one has ~L22 > max(~L21, ~R21), which leads to a contradiction.
Thus, Lemma 2.2 holds.
Lemma 2.3. Let w=kh=anrn+an−1rn−1+⋯+a1r+a0bnrn+bn−1rn−1+⋯+b1r+b0. If ˜p=˜q, ˜h≥˜k, then ˜p=˜q, ˜h=˜k, and a2n=b2n.
Proof. When ˜k=0, ˜h=1, then w=kh=cr+b, so ~L22 ≤ 5+˜p < ~L21 = 6+˜p = ~R21. Solving both sides of the coefficient of highest degree term, one gets that λ=−2, which leads to a contradiction.
When ˜k=0, ˜h≥2, then ~L22 ≤ 5˜h+˜p, ~L21 ≤ 5˜h+˜p+1 = ~R21. Let k=1, h=dnrn+dn−1rn−1+⋯+d1r+d0(n≥2), A=qp=rs+as−1rs−1+...+a1r+a0rs+bs−1rs−1+⋯+b1r+b0. Then the coefficient of highest degree term in L21 is
n(n+1)d5n, | (2.9) |
and the coefficient of highest degree term in R21 is
−λd5n. | (2.10) |
Solving the both sides of the coefficient of highest degree term, one has λ=−n(n+1)<0, which leads to a contradiction.
When ˜k=1, ˜h=1, then ~L21 ≤ 6+˜p, ~L22 ≤ 5+˜p. Let w=br+cr+a, if b2≠1, then ~R21 = 7+˜p, which leads to a contradiction. So b2=1, i.e., w2=1 (r→∞).
When ˜k=1, ˜h≥2, then ~L22 ≤ 5˜h+˜p+1, ~L21 ≤ 5˜h+˜p+2 = ~R21. Let k=ar+c, h=dnrn+dn−1rn−1+⋯+d1r+d0 (n≥2), then the coefficient of highest degree term in L21 is
n(n−1)ad5n, | (2.11) |
and the coefficient of highest degree term in R21 is
−λad5n. | (2.12) |
Solving both sides of the coefficient of highest degree term, one gets λ=−n(n−1), which leads to a contradiction.
When ˜k≥2, and w=kh=anrn+an−1rn−1+⋯+a1r+a0bmrm+bm−1rm−1+⋯+b1r+b0 (m≥n≥2), considering ˜h>˜k and m>n firstly, then ~L22 ≤ 5˜h+˜p+˜k, ~L21 ≤ 5˜h+˜p+˜k+1 = ~R21. The coefficient of highest degree term in L21 is
anb5m[2m2+n(n−1)−2nm−m(m−1)], | (2.13) |
and the coefficient of highest degree term in R21 is
−λanb5m. | (2.14) |
Solving both sides of the coefficient of highest degree term, one gets
λ=−[2m2+n(n−1)−2nm−m(m−1)]. | (2.15) |
In fact, by (2.13), one has
2m2+n(n−1)−2nm−m(m−1)=(m−n)(m−n+1)>0. | (2.16) |
So λ<0, which leads to a contradiction. If ˜h=˜k, a2n ≠ b2n, then ~L21 ≤ 6˜h+˜p, ~L22 ≤ 6˜h+˜p−1, ~R21 = 6˜h+˜p+1, which lead to a contradiction, i.e., w2=1 (r→∞).
Thus, Lemma 2.3 holds.
Lemma 2.4. The case ˜p=˜q, ˜h=˜k can not happen.
Proof. When ˜h=˜k=1, w=r+br+a, then ~L22<~L21=6+˜p=~R21, thus the coefficient of highest degree term in L21 is
2(b−a), | (2.17) |
and the coefficient of highest degree term in R21 is
2λ(b−a). | (2.18) |
Solving the both sides of the coefficient of highest degree term, we discover λ=1, which leads to a contradiction. If let w=−r+br+a, also leads to a contradiction in a same way.
For ˜h=˜k≥2, let A=rm+cm−1rm−1+⋯+c1r+c0rm+dm−1rm−1+⋯+d1r+d0, w=rn+an−1rn−1+⋯+a1r+a0rn+bn−1rn−1+⋯+b1r+b0 (w=−rn+an−1rn−1+⋯+a1r+a0rn+bn−1rn−1+⋯+b1r+b0 also leads to the same result). If an−1≠bn−1, then ~L22 ≤ 6˜h+˜p−1 < ~L21 = ~R21 = 6˜h+˜p. Solving both sides of the coefficient of highest degree term, one gets λ=1, which leads to a contradiction. So, an−1 = bn−1. If an−2 ≠ bn−2, then ~L22 ≤ 6˜h+˜p−2 < ~L21 = ~R21 = 6˜h+˜p−1. Solving both sides of the coefficient of highest degree term, one has λ=3, which leads to a contradiction. So, an−2=bn−2. This reminds us that perhaps ai=bi(i≤n−2). In the following, we use mathematical induction to prove ai=bi. With the reduction to absurdity, assume ∃ ai≠bi and ai+j=bi+j, j≥1, 0≤i<n−2. So w=kh=rn+an−1rn−1+an−2rn−2+⋯+ai+1ri+1+airi+⋯rn+an−1rn−1+an−2rn−2+⋯+ai+1ri+1+biri+⋯. By (2.6), one has
L21=(ai−bi)(i2−i+n2+n−2ni)r5n+m+i+1+⋯, | (2.19) |
L22=(i−n)(ai−bi)(dm−1−cm−1)r5n+m+i−2+⋯, | (2.20) |
R21=2λ(ai−bi)r5n+m+i+1+⋯. | (2.21) |
Solving both sides of the coefficient of highest degree term, one gets
n2+n=2ni+i−i2+2λ≤2n(n−2)+n−2−(n−2)2+2λ=n2+n+2λ−6. | (2.22) |
Thus λ≥3, which leads to a contradiction. Then w≡1, and contradicts the hypothesis. Here, if we assume w=kh=−rn+an−1rn−1+⋯+a1r+a0rn+bn−1rn−1+⋯+b1r+b0 in the beginning, we will get the result that w≡−1, which is also a contradiction.
Thus, Lemma 2.4 holds.
Lemma 2.5. The case ˜q=˜p+2, ˜k=˜h+1 can not happen.
Proof. We consider ˜h≥2 firstly. Let
w=kh=arn+1+anrn+⋯+a1r+a0rn+cn−1rn−1+⋯+c1r+c0, |
A=qp=rm+2+dm+1rm+1+⋯+d1r+d0brm+bm−1rm−1+⋯+b1r+b0, |
and b<0, then ~L21≤5˜h+˜k+˜q+1. By calculating, the corresponding coefficient of highest degree term is 0, thus ~L21≤5˜h+˜k+˜q. What's more, ~L22≤5˜h+˜k+˜q+1, and the coefficient of highest degree term in 5˜h+˜k+˜q+1 is −(a+a5b) and ~R21=5˜h+˜k+˜q+1. The corresponding coefficient is λa3b. Solving both sides of coefficient of highest degree term, one gets
a4b+λa2b+1=0. | (2.23) |
From (2.5), one gets ~L1=~L2=~L3=~R2=4˜h+2˜p+4>~R1=4˜h+2˜p+2. Comparing the coefficient of highest degree term in (L1+L2+L3)(3b+2ba2) and R2 (−a4b2), one gets
a4b+2a2+3=0. | (2.24) |
Calculating (2.23) and (2.24), one has
2λa4+(2λ+2)a2+3=0. | (2.25) |
If (2.25) has solutions, then λ≤2−√3 or λ≥2+√3, which leads to a contradiction.
If ˜h=0, then w=ar+b. This case has been discussed in the proof of Lemma 2.2. When ˜h=1, ˜k=2, we suppose w=kh=br2+b1r+b0r+c, A=arm+2+am+1rm+1+⋯+a1+a0rm+dm−1rm−1+⋯+d1r+d0, (a≠0, b≠0). Solving the coefficient of highest degree term in L21, L22, R21 and observing (2.6), one gets ~L21≤10+˜p. By calculating, the coefficient of highest degree term is 0, thus ~L21≤9+˜p. What's more, ~L22≤10+˜p, the corresponding coefficient of highest degree term is −b(a+b4), ~R21=10+˜p, the corresponding coefficient of highest degree term is λb3, then one has
b4+λb2+a=0. | (2.26) |
Observing (2.5), one gets ~L1=~L2=~L3=~R2=2m+8>~R1=2m+6. Comparing the coefficient of highest degree term in (L1+L2+L3): (3a+2ab2) and in R2: (−b4), one has
3a+2ab2+b4=0. | (2.27) |
Calculating (2.26) and (2.27), one can see that
2b4+2(1+λ)b2+3λ=0. | (2.28) |
Thus, when (2.28) has solutions, λ≤2−√3 or λ≥2+√3 holds, which leads to a contradiction.
Thus, the proof of Lemma 2.5 is completed.
By Lemma 2.1–2.5, we complete the proof of Theorem 1.1.
Remark 2.6. If we consider the case that adding the perturbed coefficient into (1.4) for the first term as follows:
ζr2Aw″+[r(1−A)−(1−w2)2r]w′+w(1−w2)=0, | (2.29) |
we can also get the same result as the conclusion in this paper. Here ζ∈(0.5,2) and ζ≠1. The proof of this result is similar to Theorem 1.1 if we add the perturbed coefficient λ into (1.4), so we omit here.
In this section, we prove the existence and uniqueness of the perturbed EYM equations. The reference [9] provides a rigorous proof of the existence and uniqueness of the solutions to the Einstein-Yang-Mills equations with gauge group SU(2). After adding the perturbed term λ to (1.4), we discover that the perturbed equations have the same properties as the original equations in existence and uniqueness.
For the definitions of C2+α(ˉr,ˉr+ε), D1, D2, D3, X, d(⋅,⋅), T, T1, T2 and T3, we still use the definitions in [9]. The main work in [9] is to prove that T1,T2 and T3 are contract mappings. By analysis, to prove our results, we just need to prove T2 is a contract mapping. Recalling u1,u2,w1,w2 in C2+α(ˉr,ˉr+ϵ), T2(w,z,A)=w′(ˉr)−∫rˉrλuw+ϕzs2Ads, and denoting θ=(w,z,A), then
T2(θ1)−T2(θ2)=∫rˉr[λu2w2s2A2−λu1w1s2A1+ϕ2z2s2A2−ϕ1z1s2A1]ds=∫rˉr[λ(u2w2−ˉuˉw)s2A2−λ(u1w1−ˉuˉw)s2A1+ϕ2z2−ˉϕˉzs2A2−ϕ1z1−ˉϕˉzs2A1+1s2(1A2−1A1)(λˉuˉw+ˉϕˉz)]ds. |
For convenience, denoting
Δf:=f1−f2 (f∈C1+α), |
then
Δ(λuw−λˉuˉws2A)=λu2w2−λˉuˉws2A2−λu1w1−λˉuˉws2A1, |
and
‖T2(θ1)−T2(θ2)‖1+α=‖Δ(λuw−λˉuˉwr2A)+Δ(ϕz−ˉϕˉzr2A)−Δ(1A)1r2(λˉuˉw+ˉϕˉz)‖α≤λ‖Δ(uw−ˉuˉwr2A)‖α+‖Δ(ϕz−ˉϕˉzr2A)‖α+‖Δ(1A)1r2(λˉuˉw+ˉϕˉz)‖α. |
Next, we estimate the above equation term by term.
For λ‖Δ(uw−ˉuˉwr2A)‖α, denoting ϱ2=r2−ˉr and by lemma 5.3 in [9], one can get
λ‖Δ(uw−ˉuˉwr2A)‖α=λr2‖u2w2A2−u1w1A2+u1w1A2−u1w1A1+ˉuˉwA1−ˉuˉwA2‖α≤λcˉr2[‖1B2‖α‖u2w2−u1w1ϱ2‖∞+‖1B2‖∞‖u2w2−u1w1ϱ2‖α]+λˉr2[‖u1w1‖α‖1A2−1A1‖∞+‖u1w1‖∞‖1A2−1A1‖α+ˉuˉw‖1A1−1A2‖α]. |
Due to u1,u2,w1,w2 in C2+α(ˉr,ˉr+ϵ), (u1w1)(ˉr)=(u2w2)(ˉr), (u1w1)′(ˉr)=(u2w2)′(ˉr), (u1w1)″(ˉr)=(u2w2)″(ˉr), then ‖Δ(uw)ϱ2‖α→0, ‖Δ(uw)ϱ2‖∞→0. Hence,
‖1B2‖α‖u2w2−u1w1ϱ2‖∞→0, ‖1B2‖∞‖u2w2−u1w1ϱ2‖α→0, | (3.1) |
as ε→0. By (1A2−1A1)(ˉr)=0,(1A2−1A1)′(ˉr)=0, ‖u1w1‖∞→0 and ‖ˉuˉw‖∞→0, one has
‖u1w1‖∞‖(1A2−1A1)‖α→0, ˉuˉw‖1A1−1A2‖α→0. | (3.2) |
as ε→0. Combining (3.1) and (3.2) to get
λ‖Δ(uw−ˉuˉwr2A)‖α→0 (ε→0). | (3.3) |
For ‖Δ(ϕz−ˉϕˉzr2A)‖α, one has
‖Δ(ϕz−ˉϕˉzr2A)‖α≤‖Δ(ϕz−ˉϕzr2A)‖α+‖(ˉϕz−ˉϕˉzr2A)‖α. |
It is easy to see ‖Δ(ϕz−ˉϕzr2A)‖α→0, as ε→0. For convenience, defining
n(r)=ˉϕz−dϱˉϕ−ˉϕˉzcr2, |
one has ni(r)=ˉϕzi−dϱˉϕ−ˉϕ¯zicr2, and
‖Δ(ˉϕz−ˉϕˉzr2A)‖α=‖n2ϱB2−n1ϱB1‖α≤‖n2ϱB2−n2ϱB1‖α+‖n2ϱB1−n1ϱB1‖α. | (3.4) |
Because n2ϱB2−n2ϱB1=n2B1B2(B1−B2ϱ), one gets
‖n2ϱB2−n2ϱB1‖α≤‖n2B1B2‖∞‖B1−B2ϱ‖α+‖n2B1B2‖α‖B1−B2ϱ‖∞. |
Due to n2B1B2∈C1+α, n2=ˉϕcr2(z2−dϱ−ˉz), then
n2(ˉr)=ˉϕcˉr2(ˉz−ˉz−dϱ). |
Because of ϱ=ˉr−ˉr=0, n2(ˉr)=0,
n′2(ˉr)=ˉϕc[1r2(z′2−d)−2r3(z2−dϱ−ˉz)](ˉr)=ˉϕc[1ˉr2(d−d)−2ˉr3(β−β−dϱ(ˉr))]=0. |
Hence (n2B1B2)(ˉr)=0,(n2B1B2)′(ˉr)=0, furthermore
‖n2B1B2‖∞→0, ‖n2B1B2‖α→0, |
and
‖n2B1B2‖∞‖B1−B2ϱ‖α→0, |
as ε→0. Due to (B2−B1ϱ)(ˉr)=0, one has
‖B2−B1ϱ‖∞≤εα‖(B2−B1)/ϱ‖α≤ϵα1+α‖B1−B2ϱ‖1+α, |
and then ε→0,
‖n2B1B2‖α‖B1−B2ϱ‖∞→0, ‖n2ϱB2−n2ϱB1‖α→0. | (3.5) |
For the last term in (3.4), denoting h(r)=ˉϕB1r2c for convenience, then
‖n2ϱB1−n1ϱB1‖α=‖ˉϕB1r2c(z2−dϱ−ˉz−z1+dϱ+ˉzϱ)‖α=‖hz2−z1ϱ‖α. |
Because h∈C1+α,h(ˉr)=ˉϕB(ˉr)ˉr2c, one has
h(ˉr)=cB(ˉr)c=11+e2cϱ(ˉr)=1, |
and (h−1)∈C1+α, (h−1)(ˉr)=h(ˉr)−1=0, ‖h−1‖∞→0. Moreover, 0<δ<α,‖h‖∞≤1+δ, then
‖n2ϱB1−n1ϱB1‖α≤‖h‖∞‖z2−z1ϱ‖α+‖h‖α‖z2−z1ϱ‖∞. |
Due to the fact that (z2−z1)(ˉr)=0 and ‖z2−z1ϱ‖≤11+α‖z2−z1‖1+α, then
‖n2ϱB1−n1ϱB1‖α≤(1+δ)11+α‖z2−z1‖1+α+‖h‖α‖z2−z1ϱ‖∞, | (3.6) |
and
‖z2−z1ϱ‖∞→0, ‖h‖α‖z2−z1ϱ‖∞→0, |
as ε→0. Let 0<k=1+δ1+α<1, then
‖n2ϱB1−n1ϱB1‖α≤k‖z2−z1‖1+α+O(ε). | (3.7) |
Furthermore, λˉuˉw+ˉϕˉz=ˉr2ˉAˉw″=0, then
‖T2(θ1)−T2(θ2)‖1+α≤k‖z2−z1‖1+α+O(ε). | (3.8) |
So T2 is a contract mapping. Thus, by Banach fixed-point theorem, in the interval ˉr≤r≤ˉr+ε, T has a unique fixed point (A(r,ˉw),w(r,ˉw),w′(r,ˉw))∈ X. This completes the proof of Theorem 1.2.
By Theorems 1.1 and 1.2, we can see that the local solution is unique. Moreover, this solution is not rational solution, but C2+α solution. This means the results in Theorem 1.3 holds. Since the current methods of finding ghost solitons are all based on the rational fraction solution, these results show that there is no rational ghost soliton solution for the EYM equation.
The authors would like to thank the referees and the editor for their valuable comments which led to improvement of this work. The authors are supported by the National Natural Science Foundation of China (Grant Nos. 12001415, 12001276, 11961080, 11561076).
All authors declare no conflicts of interest in this paper.
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