Neutrino oscillations in a variable-density medium and v-bursts due to the gravitational collapse of stars

2018 ◽  
pp. 311-314
Author(s):  
S. P. Mikheev ◽  
A. Yu. Smirnov
1986 ◽  
Vol 150 (12) ◽  
pp. 632
Author(s):  
S.P. Mikheev ◽  
A.Yu. Smirnov

2018 ◽  
Vol 852 (2) ◽  
pp. 120 ◽  
Author(s):  
L. Becerra ◽  
M. M. Guzzo ◽  
F. Rossi-Torres ◽  
J. A. Rueda ◽  
R. Ruffini ◽  
...  

1986 ◽  
Vol 29 (12) ◽  
pp. 1155-1157 ◽  
Author(s):  
Stanislav P Mikheev ◽  
A Yu Smirnov

2011 ◽  
Vol 42 (1) ◽  
pp. 119-133
Author(s):  
V. A. Komarov ◽  
A. V. Boldyrev

Author(s):  
Flavio Mercati

Shape Dynamics (SD) is a field theory that describes gravity in a different way than General Relativity (GR): it assumes a preferred notion of simultaneity, and the dynamical content of the theory consists of conformal 3- geometries. SD coincides with (GR) in most situations, in particular in the experimentally well-tested regimes, but it departs from it in some strong-gravity situations, for example at cosmological singularities or upon gravitational collapse. This chapter provides a quick introduction to the theory and a brief description of its present state.


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