论文标题
在能量空间中正弦纠结的渐近稳定性上
On the asymptotic stability of the sine-Gordon kink in the energy space
论文作者
论文摘要
我们考虑1+1维中的正弦 - 戈登(SG)方程。扭结是对SG的静态,非对称的精确解决方案,在能量空间$ h^1 \ times l^2 $中稳定。众所周知,扭结周围的线性化操作员具有简单的内核,没有内部模式。然而,它在连续频谱的底部具有奇特的共振,与(in)著名的摇摆扭结的存在密切相关,这是扭结周围SG的明确定期定期解决方案,与能量空间中扭结的渐近稳定性相矛盾。 在本文中,我们进一步研究了渐近稳定性问题中共振的影响。我们还讨论了SG环境中呼吸器,扭曲和共鸣之间的关系。通过收集Bäcklund变换(BT)和围绕真空解决方案的奇数扰动的病毒估计,我们首先确定BTS与Wobbling Kink解决方案相关的初始数据的歧管。事实证明,(甚至)小呼吸与扭结周围的奇怪扰动密切相关,包括摇摆的扭结本身。由于此结果,使用BTS,我们可以构建一个接近扭结的初始数据的平滑歧管,该数据在能量空间中存在渐近稳定性。初始数据具有形式的空间对称性(Kink + Odd,偶数),原则上没有谐振,而不是由流量保存。尽管存在SG中的扭结,但这种渐近稳定性仍然具有。我们还表明,在奇数数据下,摇摆的扭结是轨道稳定的,并在线性bäcklund变换级别上阐明了SG和$ ϕ^4 $之间的一些有趣的连接。
We consider the sine-Gordon (SG) equation in 1+1 dimensions. The kink is a static, non-symmetric exact solution to SG, stable in the energy space $H^1\times L^2$. It is well-known that the linearized operator around the kink has a simple kernel and no internal modes. However, it possesses an odd resonance at the bottom of the continuum spectrum, deeply related to the existence of the (in)famous wobbling kink, an explicit periodic-in-time solution of SG around the kink that contradicts the asymptotic stability of the kink in the energy space. In this paper, we further investigate the influence of resonances in the asymptotic stability question. We also discuss the relationship between breathers, wobbling kinks and resonances in the SG setting. By gathering Bäcklund transformations (BT) and Virial estimates around odd perturbations of the vacuum solution, we first identify the manifold of initial data around zero under which BTs are related to the wobbling kink solution. It turns out that (even) small breathers are deeply related to odd perturbations around the kink, including the wobbling kink itself. As a consequence of this result, using BTs we can construct a smooth manifold of initial data close to the kink, for which there is asymptotic stability in the energy space. The initial data has spatial symmetry of the form (kink + odd, even), non-resonant in principle, and not preserved by the flow. This asymptotic stability property holds despite the existence of wobbling kinks in SG. We also show that wobbling kinks are orbitally stable under odd data, and clarify some interesting connections between SG and $ϕ^4$ at the level of linear Bäcklund transformations.