scholarly journals Collisional interactions between self-interacting nonrelativistic boson stars: Effective potential analysis and numerical simulations

2016 ◽  
Vol 94 (6) ◽  
Author(s):  
Eric Cotner
1999 ◽  
Vol 14 (27) ◽  
pp. 4259-4274 ◽  
Author(s):  
SZE-SHIANG FENG ◽  
GUANG-JIONG NI

Using the new regularization and renormalization scheme recently proposed by Yang and used by Ni et al., we analyze the sine–Gordon and sinh–Gordon models within the framework of Gaussian effective potential in D+1 dimensions. Our analysis suffers no divergence and so does not suffer from the manipulational obscurities in the conventional analysis of divergent integrals. Our main conclusions agree exactly with those of Ingermanson for D=1,2 but disagree for D=3: the D=3 sinh(sine)–Gordon model is nontrivial. Furthermore, our analysis shows that for D=1,2, the running coupling constant (RCC) has poles for sine–Gordon model (γ2<0) and the sinh–Gordon model (γ2>0) has a possible critical point [Formula: see text] while for D=3, the RCC has poles for both γ2>0 and γ2<0.


2021 ◽  
Vol 2021 (6) ◽  
Author(s):  
Takuya Hirose ◽  
Nobuhito Maru

Abstract We study possibilities to realize a nonvanishing finite Wilson line (WL) scalar mass in flux compactification. Generalizing loop integrals in the quantum correction to WL mass at one-loop, we derive the conditions for the loop integrals and mode sums in one-loop corrections to WL scalar mass to be finite. We further guess and classify the four-point and three-point interaction terms satisfying these conditions. As an illustration, the nonvanishing finite WL scalar mass is explicitly shown in a six dimensional scalar QED by diagrammatic computation and effective potential analysis. This is the first example of finite WL scalar mass in flux compactification.


2007 ◽  
Vol 43 (1) ◽  
pp. 350-364 ◽  
Author(s):  
María F. González ◽  
Xavier Giménez ◽  
Javier González ◽  
Josep Maria Bofill

1999 ◽  
Vol 09 (01) ◽  
pp. 273-285 ◽  
Author(s):  
S. R. BISHOP ◽  
D. J. SUDOR

The planar pendulum has been used as an example of a simple oscillator for over 300 years with notable historical contributions by Galileo and Huygens. Initially interest was focused on small displacements from the stable hanging position specifically to determine the period of oscillation. More recently attention has switched to larger amplitude and chaotic motions as a consequence of periodic forcing to the pivot point. To explain experimentally observed behavior, we investigate here the existence of stable inverted solutions of a pendulum sinusoidally driven, in the first instance by a purely vertical force and then by an almost vertical force by giving a small tilt to the system. An effective potential function is considered to provide analytical justification of the numerical simulations.


2007 ◽  
Vol 21 (01) ◽  
pp. 59-68 ◽  
Author(s):  
GUENNADI A. KOUZAEV ◽  
KARL J. SAND

An Ioffe–Pritchard trap for cold dressed atoms is studied by analytical and numerical simulations. The effective potential in this trap is formed by the static magnetic and radio-frequency fields, and the minimums are formed around the current bars. The depth of the minimums and the overall topology of the effective potential are controlled electronically. The studied regime of the Ioffe–Pritchard trap is of interest for high-sensitivity cold atom interferometers.


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