scholarly journals Neutrino oscillations in strong gravitational fields

1996 ◽  
Vol 54 (2) ◽  
pp. 1587-1599 ◽  
Author(s):  
Dardo Píriz ◽  
Mou Roy ◽  
José Wudka
2011 ◽  
Vol 20 (02) ◽  
pp. 507-513 ◽  
Author(s):  
MAREK GÓŹDŹ ◽  
MAREK ROGATKO

Neutrinos do oscillate, which up to our best knowledge implies that they are massive particles. As such, neutrinos should interact with gravitational fields. As their masses are tiny, the gravitational fields must be extremely strong. In this paper we study the influence of black holes described by non-trivial topologies on the neutrino oscillations. We present approximate analytical and numerical solutions of certain specific cases.


2014 ◽  
Vol 45 (1) ◽  
pp. 234-236 ◽  
Author(s):  
Yu. N. Obukhov ◽  
A. J. Silenko ◽  
O. V. Teryaev

2010 ◽  
Vol 27 (3) ◽  
pp. 272-282 ◽  
Author(s):  
Jean-Pierre Macquart ◽  
M. Bailes ◽  
N. D. R. Bhat ◽  
G. C. Bower ◽  
J. D. Bunton ◽  
...  

AbstractWe are developing a purely commensal survey experiment for fast (<5 s) transient radio sources. Short-timescale transients are associated with the most energetic and brightest single events in the Universe. Our objective is to cover the enormous volume of transients parameter space made available by ASKAP, with an unprecedented combination of sensitivity and field of view. Fast timescale transients open new vistas on the physics of high brightness temperature emission, extreme states of matter and the physics of strong gravitational fields. In addition, the detection of extragalactic objects affords us an entirely new and extremely sensitive probe on the huge reservoir of baryons present in the IGM. We outline here our approach to the considerable challenge involved in detecting fast transients, particularly the development of hardware fast enough to dedisperse and search the ASKAP data stream at or near real-time rates. Through CRAFT, ASKAP will provide the testbed of many of the key technologies and survey modes proposed for high time resolution science with the SKA.


2011 ◽  
Vol 84 (2) ◽  
Author(s):  
Yuri N. Obukhov ◽  
Alexander J. Silenko ◽  
Oleg V. Teryaev

2009 ◽  
Vol 24 (14) ◽  
pp. 1109-1120
Author(s):  
C. A. BERTULANI ◽  
J. T. HUANG ◽  
P. G. KRASTEV

We discuss the effects of non-inertial motion in reactions occurring in laboratory, stars, and elsewhere. It is demonstrated that non-inertial effects due to large accelerations during nuclear collisions might have appreciable effects nuclear and atomic transitions. We also explore the magnitude of the corrections induced by strong gravitational fields on nuclear reactions in massive, compact stars, and the neighborhood of black holes.


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