Travelling solitary waves for boson stars

dc.contributor.authorZhang, Guoqing
dc.contributor.authorSong, Ningning
dc.date.accessioned2021-11-29T16:07:09Z
dc.date.available2021-11-29T16:07:09Z
dc.date.issued2019-05-28
dc.description.abstractIn this article, we study the pseudo-relativistic Hartree equation i∂tψ = (√-∆ + m2 - m)ψ - (e-μ|x| / 4π|x| ∗ |ψ|2)ψ, on ℝ3, which describes the dynamics of pseudo-relativistic boson stars with rest mass m > 0 in the mean-field limit. Based on Ekeland variational principle, concentration-compactness lemma and Gagliardo-Nirenberg inequality, we prove existence of travelling solitary waves under the critical stellar mass. In addition to their existence, we obtain orbital stability by using a general idea presented in Cazenave and Lions [2].
dc.description.departmentMathematics
dc.formatText
dc.format.extent12 pages
dc.format.medium1 file (.pdf)
dc.identifier.citationZhang, G., & Song, N. (2019). Travelling solitary waves for boson stars. <i>Electronic Journal of Differential Equations, 2019</i>(73), pp. 1-12.
dc.identifier.issn1072-6691
dc.identifier.urihttps://hdl.handle.net/10877/14961
dc.language.isoen
dc.publisherTexas State University, Department of Mathematics
dc.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.sourceElectronic Journal of Differential Equations, 2019, San Marcos, Texas: Texas State University and University of North Texas.
dc.subjectTravelling solitary wave
dc.subjectBoson star equation
dc.subjectCritical stellar mass
dc.titleTravelling solitary waves for boson stars
dc.typeArticle

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