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Boson Stars as Solitary Waves
Authors:Jürg Fröhlich  B Lars G Jonsson  Enno Lenzmann
Institution:(1) Institute for Theoretical Physics, ETH Zurich, 8093 Zurich, Switzerland;(2) Division of Electromagnetic Engineering, School of Electrical Engineering, Royal Insitute of Technology, SE-100 44 Stockholm, Sweden;(3) Department of Mathematics, ETH Zurich, 8092 Zurich, Switzerland;(4) Department of Mathematics, MIT, Cambridge, MA 02139, USA
Abstract:We study the nonlinear equation
$$i \partial_t \psi = (\sqrt{-\Delta + m^2} - m)\psi - ( |x|^{-1} \ast |\psi|^2 ) \psi \quad {\rm on}\,\mathbb{R}^3$$
which is known to describe the dynamics of pseudo-relativistic boson stars in the mean-field limit. For positive mass parameters, m >  0, we prove existence of travelling solitary waves, $$\psi(t,x) = e^{{i}{t}\mu} \varphi_{v}(x - vt)$$ , for some $$\mu \in {\mathbb{R}}$$ and with speed |v| <  1, where c = 1 corresponds to the speed of light in our units. Due to the lack of Lorentz covariance, such travelling solitary waves cannot be obtained by applying a Lorentz boost to a solitary wave at rest (with v =  0). To overcome this difficulty, we introduce and study an appropriate variational problem that yields the functions $$\varphi_v \in {\bf H}^{1/2}({\mathbb{R}}^3)$$ as minimizers, which we call boosted ground states. Our existence proof makes extensive use of concentration-compactness-type arguments. In addition to their existence, we prove orbital stability of travelling solitary waves $$\psi(t, x) = e^{{i}{t}\mu}\varphi_v(x - vt)$$ and pointwise exponential decay of $$\varphi_v(x)$$ in x.
Keywords:
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