Effective masses in Sn‐doped Ga1−xAlxAs (x<0.33) determined by the Shubnikov–de Haas effect

1985 ◽  
Vol 58 (9) ◽  
pp. 3481-3484 ◽  
Author(s):  
B. El Jani ◽  
P. Gibart ◽  
J. C. Portal ◽  
R. L. Aulombard
Keyword(s):  
Effective Masses ◽  
Haas Effect

Fermi surface, effective masses, and Dingle temperatures ofZrTe5as derived from the Shubnikov–de Haas effect

1985 ◽  
Vol 31 (12) ◽  
pp. 7617-7623 ◽  
Author(s):  
G. N. Kamm ◽  
D. J. Gillespie ◽  
A. C. Ehrlich ◽  
T. J. Wieting ◽  
F. Levy
Keyword(s):  
Fermi Surface ◽  
Effective Masses ◽  
Haas Effect

Erratum: Fermi surface, effective masses, and Dingle temperatures of ZrTe5as derived from the Shubnikov-de Haas effect

1986 ◽  
Vol 33 (12) ◽  
pp. 8791-8791
Author(s):  
G. N. Kamm ◽  
D. J. Gillespie ◽  
A. C. Ehrlich ◽  
T. J. Wieting ◽  
F. Levy
Keyword(s):  
Fermi Surface ◽  
Effective Masses ◽  
Haas Effect

Fermi surface, effective masses, and energy bands of HfTe_{5} as derived from the Shubnikov–de Haas effect

1987 ◽  
Vol 35 (3) ◽  
pp. 1223-1229 ◽  
Author(s):  
G. Kamm ◽  
D. Gillespie ◽  
A. Ehrlich ◽  
D. Peebles ◽  
F. Levy
Keyword(s):  
Fermi Surface ◽  
Energy Bands ◽  
Effective Masses ◽  
Haas Effect

On the history of the Einstein–de Haas effect

1979 ◽  
Vol 128 (7) ◽  
pp. 545 ◽  
Author(s):  
Viktor Ya. Frenkel'
Keyword(s):  
History Of ◽  
Haas Effect

Effective masses in a dense fermion background — Applied to neutrinos, dark matter and dark energy

2014 ◽  
Vol 29 (21) ◽  
pp. 1444010
Author(s):  
Bruce H. J. McKellar ◽  
T. J. Goldman ◽  
G. J. Stephenson
Keyword(s):  
Dark Matter ◽  
Dark Energy ◽  
Scalar Field ◽  
Effective Mass ◽  
Negative Pressure ◽  
Expectation Value ◽  
Effective Masses ◽  
Neutrino Astrophysics

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.

Anisotropy of effective masses induced by strain in Janus MoSSe and WSSe monolayers

2021 ◽  
pp. 114826
Author(s):  
M. Farkous ◽  
M. El-Yadri ◽  
H. Erguig ◽  
L.M. Pérez ◽  
D. Laroze ◽  
...  
Keyword(s):  
Effective Masses
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