möbius inverse
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2015 ◽  
Vol 186 ◽  
pp. 7-12 ◽  
Author(s):  
Michel Grabisch ◽  
Pedro Miranda

2005 ◽  
Vol 1 (3) ◽  
pp. 211-217 ◽  
Author(s):  
Antoine Billot ◽  
Jacques-Francois Thisse
Keyword(s):  

2002 ◽  
Vol 17 (21) ◽  
pp. 1377-1381 ◽  
Author(s):  
HARET C. ROSU ◽  
MICHEL PLANAT

Micron-sized black holes do not necessarily have a constant horizon temperature distribution. The black hole remote-sensing problem means to find out the "surface" temperature distribution of a small black hole from the spectral measurement of its (Hawking) grey pulse. This problem has been previously considered by Rosu, who used Chen's modified Möbius inverse transform. Here, we hint on a Ramanujan generalization of Chen's modified Möbius inverse transform that may be considered as a special wavelet processing of the remote-sensed grey signal coming from a black hole or any other distant grey source.


2000 ◽  
Vol 62 (3) ◽  
pp. R3019-R3022 ◽  
Author(s):  
DengMing Ming ◽  
Tao Wen ◽  
JiXin Dai ◽  
Xianxi Dai ◽  
William E. Evenson

1998 ◽  
Vol 13 (09) ◽  
pp. 695-699 ◽  
Author(s):  
HARET C. ROSU

This is a short note on the black hole remote-sensing problem, i.e. finding out "surface" temperature distributions of various types of small (micron-sized) black holes from the spectral measurements of their Hawking grey pulses. Chen's modified Möbius inverse transform is illustrated in this context.


1998 ◽  
Vol 200 (2) ◽  
pp. 428-438 ◽  
Author(s):  
Mark V. Lawson

1993 ◽  
Vol 108 (12) ◽  
pp. 1333-1339 ◽  
Author(s):  
H. Rosu

1992 ◽  
Vol 168 (5-6) ◽  
pp. 378-382 ◽  
Author(s):  
Wenji Deng ◽  
Youyan Liu
Keyword(s):  

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