External field effect on the critical behavior of the interface between fluid phases

1989 ◽  
Vol 10 (2) ◽  
pp. 321-331 ◽  
Author(s):  
M. Knackstedt ◽  
M. Robert
Keyword(s):  
External Field ◽  
Critical Behavior ◽  
Field Effect ◽  
Fluid Phases

The external field effect on transient radiation of an ultrarelativistic particle

2002 ◽  
Vol 95 (5) ◽  
pp. 861-863
Author(s):  
M. I. Ryazanov
Keyword(s):  
External Field ◽  
Field Effect ◽  
Transient Radiation

External Field Effect on the Confined Dynamics in One Dimension

2018 ◽  
Vol 39 (2) ◽  
pp. 257-260
Author(s):  
Hyojoon Kim ◽  
Joung-Hahn Yoon
Keyword(s):  
External Field ◽  
Field Effect ◽  
One Dimension ◽  
Confined Dynamics

scholarly journals Testing the Strong Equivalence Principle: Detection of the External Field Effect in Rotationally Supported Galaxies

2020 ◽  
Vol 904 (1) ◽  
pp. 51
Author(s):  
Kyu-Hyun Chae ◽  
Federico Lelli ◽  
Harry Desmond ◽  
Stacy S. McGaugh ◽  
Pengfei Li ◽  
...  
Keyword(s):  
External Field ◽  
Equivalence Principle ◽  
Field Effect ◽  
Strong Equivalence Principle

scholarly journals External Field Effect on Electronic and Vibrational Properties of Carotenoids

2018 ◽  
Author(s):  
Nan Gong ◽  
Zuowei Li ◽  
Chenglin Sun ◽  
Zhiwei Men
Keyword(s):  
External Field ◽  
Field Effect ◽  
Vibrational Properties

scholarly journals Predicted MOND velocity dispersions for a catalog of ultra-diffuse galaxies in group environments

2019 ◽  
Vol 623 ◽  
pp. A36 ◽  
Author(s):  
Oliver Müller ◽  
Benoit Famaey ◽  
Hongsheng Zhao
Keyword(s):  
Dark Matter ◽  
External Field ◽  
Field Effect ◽  
Velocity Dispersion ◽  
A Priori ◽  
Three Dimensional ◽  
The Galaxy ◽  
Lower Limits ◽  
Group Environments

The possibility that ultra-diffuse galaxies are lacking dark matter has recently stimulated interest to check the validity of modified Newton dynamics (MOND) predictions on the scale of such galaxies. It has been shown that the external field effect (EFE) induced by the close-by galaxy can suppress the velocity dispersion of these systems, so that they appear almost dark matter free in the Newtonian context. Here, following up on this, we are making a priori predictions for the velocity dispersion of 22 ultra-diffuse galaxies in the nearby Universe. This sample can be used to test MOND and the EFE with future follow-up measurements. We have constructed a catalog of nearby ultra-diffuse galaxies in galaxy group environments, and set upper and lower limits for the possible velocity dispersion allowed in MOND, taking into account possible variations in the mass-to-light ratio of the dwarf and in the distance to the galaxy group. The prediction for the velocity dispersion is made as a function of the three dimensional separation of the dwarf to its host. In 17 out of 22 cases, the EFE plays a crucial role in the prediction.

scholarly journals External field effect of modified Newtonian dynamics in the Solar system

2011 ◽  
Vol 412 (4) ◽  
pp. 2530-2542 ◽  
Author(s):  
Luc Blanchet ◽  
Jérôme Novak
Keyword(s):  
Solar System ◽  
External Field ◽  
Field Effect ◽  
Modified Newtonian Dynamics ◽  
Newtonian Dynamics

scholarly journals Consequences of the external field effect for MOND disc galaxies in galaxy clusters

2018 ◽  
Vol 480 (4) ◽  
pp. 5362-5379 ◽  
Author(s):  
G N Candlish ◽  
R Smith ◽  
Y Jaffé ◽  
A Cortesi
Keyword(s):  
External Field ◽  
Galaxy Clusters ◽  
Field Effect ◽  
Disc Galaxies

scholarly journals On the MOND external field effect in the solar system

2009 ◽  
Vol 323 (3) ◽  
pp. 215-219 ◽  
Author(s):  
Lorenzo Iorio
Keyword(s):  
Solar System ◽  
External Field ◽  
Field Effect
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