4.7 Article

Kink-antikink collisions in a weakly interacting φ4 model

期刊

PHYSICAL REVIEW E
卷 102, 期 6, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevE.102.062214

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资金

  1. Ministry of Education, Culture, and Sports, Spain [FPA2017-83814-P]
  2. Xunta de Galicia [INCITE09.296.035PR]
  3. Spanish Consolider Program Ingenio 2010 CPAN [CSD2007-00042]
  4. Maria de Maetzu Unit of Excellence [MDM-2016-0692]
  5. FEDER
  6. National Science Centre, Poland [2019/03/X/ST2/01690]
  7. Polish National Science Centre [NCN 2019/35/B/ST2/00059]
  8. Xunta de Galicia (Conselleria de Educacion)

向作者/读者索取更多资源

Kink-antikink scattering in nonintegrable field theories like phi(4) theory is still rather poorly understood beyond brute-force numerical calculations, even after several decades of investigation. Recently, however, some progress has been made based on the introduction of certain self-dual background fields in these field theories which imply both the existence of static kink-antikink solutions of the Bogomol'nyi type and the possibility of an adiabatic scattering (moduli space approximation). Here we continue and generalize these investigations by introducing a one-parameter family of models interpolating between the Bogomol'nyi-Prasad-Sommerfield (BPS) model with the self-dual background field and the original phi(4) theory. More concretely, we study kink-antikink scattering in a parameter range between the limit of no static force (BPS limit) and the regime where the static interaction between kink and antikink is small (non-BPS regime). This allows us to study the impact of the strength of the intersoliton static force on the soliton dynamics. In particular, we analyze how the transition of a bound mode through the mass threshold affects the soliton dynamics in a generic process, i.e., when a static intersoliton force shows up. We show that the thin, precisely localized spectral wall which forms in the limit of no static force broadens in a well-defined manner when a static force is included, giving rise to what we call a thick spectral wall. This phenomenon results from the appearance of a stationary saddle point solution where the acceleration of the solitons owing to the attractive force is compensated by the dynamics of the sufficiently excited mode. Thus, this barrier shows up before the mode crosses the mass threshold.

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