The effective mass of excess electrons in condensed xenon: Toward methods for modeling metal-dielectric interfaces

1997 ◽  
Vol 107 (6) ◽  
pp. 1922-1930 ◽  
Author(s):  
H. F. Bowen ◽  
Brian Space
1991 ◽  
Vol 94 (9) ◽  
pp. 6132-6134 ◽  
Author(s):  
B. Plenkiewicz ◽  
Y. Frongillo ◽  
P. Plenkiewicz ◽  
J.‐P. Jay‐Gerin

1992 ◽  
Vol 97 (10) ◽  
pp. 7849-7850
Author(s):  
B. Plenkiewicz ◽  
Y. Frongillo ◽  
J.‐P. Jay‐Gerin ◽  
Ashok Jain

Author(s):  
B. Plenkiewicz ◽  
P. Plenkiewicz ◽  
J.-P. Jay-Gerin

1991 ◽  
Vol 43 (12) ◽  
pp. 7061-7063 ◽  
Author(s):  
B. Plenkiewicz ◽  
Y. Frongillo ◽  
P. Plenkiewicz ◽  
J.-P. Jay-Gerin

1993 ◽  
Vol 140 (5) ◽  
pp. 385 ◽  
Author(s):  
T.J. Lewis ◽  
J.P. Llewellyn ◽  
M.J. van der Sluijs

2011 ◽  
Vol 35 (1) ◽  
pp. 15-27
Author(s):  
Zoran Ivić ◽  
Željko Pržulj

Adiabatic large polarons in anisotropic molecular crystals We study the large polaron whose motion is confined to a single chain in a system composed of the collection of parallel molecular chains embedded in threedimensional lattice. It is found that the interchain coupling has a significant impact on the large polaron characteristics. In particular, its radius is quite larger while its effective mass is considerably lighter than that estimated within the one-dimensional models. We believe that our findings should be taken into account for the proper understanding of the possible role of large polarons in the charge and energy transfer in quasi-one-dimensional substances.


1988 ◽  
Vol 24 (1) ◽  
pp. 64-65 ◽  
Author(s):  
A. Aishima ◽  
Y. Fukushima
Keyword(s):  

2014 ◽  
Vol 29 (21) ◽  
pp. 1444010
Author(s):  
Bruce H. J. McKellar ◽  
T. J. Goldman ◽  
G. J. Stephenson

If fermions interact with a scalar field, and there are many fermions present the scalar field may develop an expectation value and generate an effective mass for the fermions. This can lead to the formation of fermion clusters, which could be relevant for neutrino astrophysics and for dark matter astrophysics. Because this system may exhibit negative pressure, it also leads to a model of dark energy.


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