Research article

Two-uniqueness of rational ghost soliton solution and well-posedness of perturbed Einstein-Yang-Mills equations

  • Received: 08 May 2021 Accepted: 12 August 2021 Published: 19 August 2021
  • MSC : 53C25, 53C26, 58J60

  • 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+A1dr2+r2(dθ2+sin2θdϕ2), (1.1)

    and the SU(2) Yang-Mills curvature 2-form is

    F=wτ1drdθ+wτ2(sinθdϕ)(1w2)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+2w2)A=1(1w2)2r2, (1.3)
    r2Aw+[r(1A)(1w2)2r]w+w(1w2)=0, (1.4)

    and

    CC=2w2r. (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+2w2)A=1(1w2)2r2, (1.6)
    r2Aw+[r(1A)(1w2)2r]w+λw(1w2)=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(1ˉw2)=0,

    where Φ(ˉr)=ˉr(1ˉw2)2ˉr0. 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 |rˉr|<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+an1rn1++a1r+a0bmrm+bm1rm1++b1r+b0, (2.1)
    w=csrs+cs1rs1++c1r+c0dtrt+dt1rt1++d1r+d0, (2.2)

    where ai, bi, ci, di (i[1,n],n1) 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 λ1, then (1.6) and (1.7) can be simplified as

    h4r3(qppq)+ph4r2q+2pqr2(khhk)2=p2h4r2p2(h2k2)2, (2.5)
    r3h2q(kh3hkh22kh2h+2hkh2)+(khkh)[pr2h4qr2h4p(h2k2)2]=λprkh3(k2h2). (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(qppq), L2=ph4r2q, L3=2pqr2(khhk)2, R1=p2h4r2, R2=p2(h2k2)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(kh3hkh22kh2h+2hkh2), L22=(khkh)[pr2h4qr2h4p(h2k2)2], R21=λprkh3(k2h2) 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., A0, then, from (1.6) and (1.7), w0, r=1 or w21, r=0.

    When k=0, i.e., w0, 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 A1 and w21.

    When h and k are constants, i.e., w is a constant, then w21 from (1.6) and (1.7), which is corresponding to Schwarzschild Solution.

    Next, we discuss the case k0, q0, 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 qppq0, then A0; If khhk0, then w0; If h2=k2, then w21. Then in the following discussion, each terms in (2.5) can not be constant except R2. Noted that

    L1:4˜h+˜p+˜q+24˜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˜p2˜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 ~L34˜h+˜p+˜q2<~L1 = ~L2 = 4˜h+˜p+˜q+2, ~R24˜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 nm>0 (an0, bm0, cs0, dt0), then the coefficient of highest degree in (L1+L2) is

    d4tanbm(nm+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 nm=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+an1rn1++a1r+a0bmrm+bm1rm1++b1r+b0,
    w=ct+1rt+1+ctrt++c1r+c0dtrt+dt1rt1++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, a0, by using coefficient of variation method to (1.6), one can see the expression of A as follows.

    If a212, then

    A=1+4ab2a2(b21)2a2+1a42a2+3r24a3b2a2+2r4ab(b21)2a2r(b21)2(2a21)r2+cr2a2+1,

    where c is a constant. Then we generate the results into (1.7) and discover the fact that

    (a52a2+3a5λa3)r3+(4a4b2a2+24a4b3λa2b)r2+a(2a2b24ab2a2+14ab2a2b2+2a2+λ3λb2)r+a[(b21)22a21(b21)2]r1acr2a2+λ(4a21)(bb3)=0. For (a52a2+3a5λa3)=0 has solutions, one has λ23 or λ2+3, which leads to a contradiction.

    If a2=12, then

    A=2+4abb22116r223abr4ab(b21)r(b21)2lnrr2+cr2,

    where c is a constant. Then we generate the results into (1.7) and discover the fact that a(3+8λ)16r3b(4+9λ)6r2+[(123λ)ab23b+(1+λ)a]r+a(b21)2(lnr1)r1acr+λ(bb3)=0. Let the coefficient of r3 be 0, one gets λ=38, which leads to a contradiction.

    When ˜h=0, ˜k2, then ~L21=˜k+˜q+1, ~L22=5˜k+˜p1, ~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˜p4, i.e., ˜k˜h2, 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 ˜h2, if ˜q˜p4, i.e., ˜k˜h2, then ~L21 5˜h+1+˜k+˜q, ~L22 = 5˜k+˜h+˜p1, ~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+an1rn1++a1r+a0bnrn+bn1rn1++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, ˜h2, then ~L22 5˜h+˜p, ~L21 5˜h+˜p+1 = ~R21. Let k=1, h=dnrn+dn1rn1++d1r+d0(n2), A=qp=rs+as1rs1+...+a1r+a0rs+bs1rs1++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 b21, then ~R21 = 7+˜p, which leads to a contradiction. So b2=1, i.e., w2=1 (r).

    When ˜k=1, ˜h2, then ~L22 5˜h+˜p+1, ~L21 5˜h+˜p+2 = ~R21. Let k=ar+c, h=dnrn+dn1rn1++d1r+d0 (n2), then the coefficient of highest degree term in L21 is

    n(n1)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(n1), which leads to a contradiction.

    When ˜k2, and w=kh=anrn+an1rn1++a1r+a0bmrm+bm1rm1++b1r+b0 (mn2), 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(n1)2nmm(m1)], (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(n1)2nmm(m1)]. (2.15)

    In fact, by (2.13), one has

    2m2+n(n1)2nmm(m1)=(mn)(mn+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+˜p1, ~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(ba), (2.17)

    and the coefficient of highest degree term in R21 is

    2λ(ba). (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=˜k2, let A=rm+cm1rm1++c1r+c0rm+dm1rm1++d1r+d0, w=rn+an1rn1++a1r+a0rn+bn1rn1++b1r+b0 (w=rn+an1rn1++a1r+a0rn+bn1rn1++b1r+b0 also leads to the same result). If an1bn1, then ~L22 6˜h+˜p1 < ~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, an1 = bn1. If an2 bn2, then ~L22 6˜h+˜p2 < ~L21 = ~R21 = 6˜h+˜p1. Solving both sides of the coefficient of highest degree term, one has λ=3, which leads to a contradiction. So, an2=bn2. This reminds us that perhaps ai=bi(in2). In the following, we use mathematical induction to prove ai=bi. With the reduction to absurdity, assume aibi and ai+j=bi+j, j1, 0i<n2. So w=kh=rn+an1rn1+an2rn2++ai+1ri+1+airi+rn+an1rn1+an2rn2++ai+1ri+1+biri+. By (2.6), one has

    L21=(aibi)(i2i+n2+n2ni)r5n+m+i+1+, (2.19)
    L22=(in)(aibi)(dm1cm1)r5n+m+i2+, (2.20)
    R21=2λ(aibi)r5n+m+i+1+. (2.21)

    Solving both sides of the coefficient of highest degree term, one gets

    n2+n=2ni+ii2+2λ2n(n2)+n2(n2)2+2λ=n2+n+2λ6. (2.22)

    Thus λ3, which leads to a contradiction. Then w1, and contradicts the hypothesis. Here, if we assume w=kh=rn+an1rn1++a1r+a0rn+bn1rn1++b1r+b0 in the beginning, we will get the result that w1, 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 ˜h2 firstly. Let

    w=kh=arn+1+anrn++a1r+a0rn+cn1rn1++c1r+c0,
    A=qp=rm+2+dm+1rm+1++d1r+d0brm+bm1rm1++b1r+b0,

    and b<0, then ~L215˜h+˜k+˜q+1. By calculating, the corresponding coefficient of highest degree term is 0, thus ~L215˜h+˜k+˜q. What's more, ~L225˜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 λ23 or λ2+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+dm1rm1++d1r+d0, (a0, b0). Solving the coefficient of highest degree term in L21, L22, R21 and observing (2.6), one gets ~L2110+˜p. By calculating, the coefficient of highest degree term is 0, thus ~L219+˜p. What's more, ~L2210+˜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, λ23 or λ2+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(1A)(1w2)2r]w+w(1w2)=0, (2.29)

    we can also get the same result as the conclusion in this paper. Here ζ(0.5,2) and ζ1. 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[λu2w2s2A2λu1w1s2A1+ϕ2z2s2A2ϕ1z1s2A1]ds=rˉr[λ(u2w2ˉuˉw)s2A2λ(u1w1ˉuˉw)s2A1+ϕ2z2ˉϕˉzs2A2ϕ1z1ˉϕˉzs2A1+1s2(1A21A1)(λˉuˉw+ˉϕˉz)]ds.

    For convenience, denoting

    Δf:=f1f2   (fC1+α),

    then

    Δ(λuwλˉuˉws2A)=λu2w2λˉuˉws2A2λu1w1λˉuˉws2A1,

    and

    T2(θ1)T2(θ2)1+α=Δ(λuwλˉuˉwr2A)+Δ(ϕzˉϕˉzr2A)Δ(1A)1r2(λˉuˉw+ˉϕˉz)αλΔ(uwˉuˉwr2A)α+Δ(ϕzˉϕˉzr2A)α+Δ(1A)1r2(λˉuˉw+ˉϕˉz)α.

    Next, we estimate the above equation term by term.

    For λΔ(uwˉuˉwr2A)α, denoting ϱ2=r2ˉr and by lemma 5.3 in [9], one can get

    λΔ(uwˉuˉwr2A)α=λr2u2w2A2u1w1A2+u1w1A2u1w1A1+ˉuˉwA1ˉuˉwA2αλcˉr2[1B2αu2w2u1w1ϱ2+1B2u2w2u1w1ϱ2α]+λˉr2[u1w1α1A21A1+u1w11A21A1α+ˉuˉw1A11A2α].

    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)ϱ2α0, Δ(uw)ϱ20. Hence,

    1B2αu2w2u1w1ϱ20,             1B2u2w2u1w1ϱ2α0, (3.1)

    as ε0. By (1A21A1)(ˉr)=0,(1A21A1)(ˉr)=0, u1w10 and ˉuˉw0, one has

    u1w1(1A21A1)α0,               ˉuˉw1A11A2α0. (3.2)

    as ε0. Combining (3.1) and (3.2) to get

    λΔ(uwˉuˉwr2A)α0    (ε0). (3.3)

    For Δ(ϕzˉϕˉzr2A)α, one has

    Δ(ϕzˉϕˉzr2A)αΔ(ϕzˉϕzr2A)α+(ˉϕzˉϕˉzr2A)α.

    It is easy to see Δ(ϕzˉϕzr2A)α0, as ε0. For convenience, defining

    n(r)=ˉϕzdϱˉϕˉϕˉzcr2,

    one has ni(r)=ˉϕzidϱˉϕˉϕ¯zicr2, and

    Δ(ˉϕzˉϕˉzr2A)α=n2ϱB2n1ϱB1αn2ϱB2n2ϱB1α+n2ϱB1n1ϱB1α. (3.4)

    Because n2ϱB2n2ϱB1=n2B1B2(B1B2ϱ), one gets

    n2ϱB2n2ϱB1αn2B1B2B1B2ϱα+n2B1B2αB1B2ϱ.

    Due to n2B1B2C1+α, n2=ˉϕcr2(z2dϱˉz), then

    n2(ˉr)=ˉϕcˉr2(ˉzˉzdϱ).

    Because of ϱ=ˉrˉr=0, n2(ˉr)=0,

    n2(ˉr)=ˉϕc[1r2(z2d)2r3(z2dϱˉz)](ˉr)=ˉϕc[1ˉr2(dd)2ˉr3(ββdϱ(ˉr))]=0.

    Hence (n2B1B2)(ˉr)=0,(n2B1B2)(ˉr)=0, furthermore

    n2B1B20,          n2B1B2α0,

    and

    n2B1B2B1B2ϱα0,

    as ε0. Due to (B2B1ϱ)(ˉr)=0, one has

    B2B1ϱεα(B2B1)/ϱαϵα1+αB1B2ϱ1+α,

    and then ε0,

    n2B1B2αB1B2ϱ0,        n2ϱB2n2ϱB1α0. (3.5)

    For the last term in (3.4), denoting h(r)=ˉϕB1r2c for convenience, then

    n2ϱB1n1ϱB1α=ˉϕB1r2c(z2dϱˉzz1+dϱ+ˉzϱ)α=hz2z1ϱα.

    Because hC1+α,h(ˉr)=ˉϕB(ˉr)ˉr2c, one has

    h(ˉr)=cB(ˉr)c=11+e2cϱ(ˉr)=1,

    and (h1)C1+α, (h1)(ˉr)=h(ˉr)1=0, h10. Moreover, 0<δ<α,h1+δ, then

    n2ϱB1n1ϱB1αhz2z1ϱα+hαz2z1ϱ.

    Due to the fact that (z2z1)(ˉr)=0 and z2z1ϱ11+αz2z11+α, then

    n2ϱB1n1ϱB1α(1+δ)11+αz2z11+α+hαz2z1ϱ, (3.6)

    and

    z2z1ϱ0,             hαz2z1ϱ0,

    as ε0. Let 0<k=1+δ1+α<1, then

    n2ϱB1n1ϱB1αkz2z11+α+O(ε). (3.7)

    Furthermore, λˉuˉw+ˉϕˉz=ˉr2ˉAˉw=0, then

    T2(θ1)T2(θ2)1+αkz2z11+α+O(ε). (3.8)

    So T2 is a contract mapping. Thus, by Banach fixed-point theorem, in the interval ˉrrˉr+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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