scholarly journals Absolute Negative Conductivity and Spontaneous Current Generation in Semiconductor Superlattices with Hot Electrons

2000 ◽  
Vol 85 (6) ◽  
pp. 1302-1305 ◽  
Author(s):  
Ethan H. Cannon ◽  
Feodor V. Kusmartsev ◽  
Kirill N. Alekseev ◽  
David K. Campbell
1991 ◽  
Vol 34 (6) ◽  
pp. 559-564 ◽  
Author(s):  
M.V. Burtyka ◽  
O.V. Glukhov ◽  
V.M. Yakovenko

2000 ◽  
Vol 27 (5-6) ◽  
pp. 495-498 ◽  
Author(s):  
Ethan H. Cannon ◽  
Feodor V. Kusmartsev ◽  
Kirill N. Alekseev ◽  
David K. Campbell

1997 ◽  
Vol 161 ◽  
pp. 711-717 ◽  
Author(s):  
John W. Dreher ◽  
D. Kent Cullers

AbstractWe develop a figure of merit for SETI observations which is anexplicitfunction of the EIRP of the transmitters, which allows us to treat sky surveys and targeted searches on the same footing. For each EIRP, we calculate the product of terms measuring the number of stars within detection range, the range of frequencies searched, and the number of independent observations for each star. For a given set of SETI observations, the result is a graph of merit versus transmitter EIRP. We apply this technique to several completed and ongoing SETI programs. The results provide a quantitative confirmation of the expected qualitative difference between sky surveys and targeted searches: the Project Phoenix targeted search is good for finding transmitters in the 109to 1014W range, while the sky surveys do their best at higher powers. Current generation optical SETI is not yet competitive with microwave SETI.


1981 ◽  
Vol 42 (C7) ◽  
pp. C7-215-C7-220 ◽  
Author(s):  
V. Bareikis ◽  
A. Galdikas ◽  
R. Miliu¡yté ◽  
J. Pozhela ◽  
Viktoravičius
Keyword(s):  

1981 ◽  
Vol 42 (C7) ◽  
pp. C7-117-C7-122 ◽  
Author(s):  
R. Brunetti ◽  
C. Jacoboni ◽  
L. Reggiani
Keyword(s):  

1984 ◽  
Vol 45 (C5) ◽  
pp. C5-131-C5-137 ◽  
Author(s):  
M. V. Klein ◽  
C. Colvard ◽  
R. Fischer ◽  
H . Morkoç

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