Stable regular solution of Einstein-Yang-Mills equation Yuewen Chen1and Shing-Tung Yau1 2 3y 1Yau Mathematical Sciences Center Tsinghua University Beijing 100084 China

2025-05-03 0 0 385.76KB 4 页 10玖币
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Stable regular solution of Einstein-Yang-Mills equation
Yuewen Chen1, and Shing-Tung Yau1, 2, 3,
1Yau Mathematical Sciences Center, Tsinghua University, Beijing 100084, China
2Yanqi Lake Beijing Institute of Mathematical Sciences and Applications, Beijing 101408, China
3Department of Mathematics, Harvard University, Cambridge, MA 02138, USA
(Dated: November 1, 2022)
In this letter, we find the first dynamically stable non-singular solution of spherically symmetric
SU(2) Einstein-Yang-Mills equation. This solution is regular at r= 0 and asymptotically flat. Since
the Yang-Mills field strength decay exponentially, the Einstein-Yang-Mills particle perhaps can be
used as a candidate for dark matter.
INTRODUCTION
In 1988, a global nontrivial static nonsingular particle-
like solution of coupled Einstein-Yang-Mills (EYM) equa-
tion was found by Bartnik and McKinnon numerically [1].
It aroused a great of interest in GR community. It was
established rigorously by Smoller-Wasserman-Yau et.al
[24]. It was also found there is an infinite black solu-
tions different coupling constants. Since it violated the
familiar no hair theorem, much excitement was gener-
ated. However, it was soon demonstrated by Strauumen-
Zhou [5] that these solutions are not dynamically stable
and therefore not physical. In this letter, we find the
first dynamically stable non singular solution of Einstein-
Yang-Mills. Since the field strength of Yang Mills of our
solution decay exponentially, we believe such particle so-
lution can be a potential candidate for dark matter.
After Bartnik-McKinnon’s pioneering work, a large
number of soliton and black hole solutions of spherically
symmetric EYM equations were found [68]. The crit-
ical behavior of spherically symmetric collapse of EYM
equations were studied in [912]. Smoller and Yau et.al
proved rigorously that the SU (2) EYM equations admit
an infinite family of black-hole solutions with a regular
event horizon [13]. However, the colored black hole found
numerically by Bizon is also unstable[14,15]. The non-
linear stability was studied in [16] and the work provided
numerical evidence for the instability of the colored black
hole solutions.
The new idea in this letter, is to study the evolution
of the time dependent EYM equation rather than only
studying the static equation [1]. Our main new result is
the observation that for suitable initial data, the EYM
equations would have a non trivial steady state solution.
Furthermore, we show this solution is stable under linear
perturbation. We write the spherically symmetric metric
as
ds2=Ae2Qdt2+1
Adr2+r2d2.
The Yang-Mills curvature tensor is given by
F=Wtτ1dt +Wtτ2dt sin θ+W0τ1dr
+W0τ2dr sin θ(1 W2)τ3sin θdφ,
where τiare the Pauli matrices. The evolution version of
Einstein-Yang-Mills equation are given by
(1
AeQWt)t= (AeQWr)r
+eQ
r2W(1 W2),
(1)
At=4
rWtWrA, (2)
rAr+A(1 + 2(W2
r+1
A2e2QW2
t)) = 1 1
r2(1 W2)2,
(3)
rQr= 2(W2
r+1
A2e2QW2
t).
(4)
We need a new coordinate transformation
x= ln(r).
We define the auxiliary functions , S, α, θ, q and c, re-
spectively, as follows
= 2(W2
r+1
A2e2QW2
t),(5)
S= 1 1
r2(1 W2)2,(6)
α=eQ,(7)
θx=,(8)
qx= 1 + ,(9)
c=Aα. (10)
To evolution Einstein-Yang-Mills system, we choose
equations (1), (3) and (4). Then, we rewrite the EYM
system as
c(1
cWt)t=c
r(c
rWx)x+
r2W(1 W2),(11)
(Aeq)x=Seq,(12)
(αeθ)x= 0.(13)
arXiv:2210.09861v3 [gr-qc] 30 Oct 2022
摘要:

StableregularsolutionofEinstein-Yang-MillsequationYuewenChen1,andShing-TungYau1,2,3,y1YauMathematicalSciencesCenter,TsinghuaUniversity,Beijing100084,China2YanqiLakeBeijingInstituteofMathematicalSciencesandApplications,Beijing101408,China3DepartmentofMathematics,HarvardUniversity,Cambridge,MA02138,U...

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