A new simulation of the EPR-Bohm correlations
Posted: Thu Jun 04, 2015 4:35 am
Hi Everyone,
I have produced yet another simulation for the EPR-Bohm correlations which is more satisfactory and faithful to my 3-sphere model than previous attempts by myself and others. But before I describe it I want to thank Fred Diether, Michel Fodje, and Albert Jan Wonnink for ongoing discussions and help, as well as to some annoying, cynical, and persistent critics (such as Richard Gill) for keeping me on my toes about this.
So, without further ado, here is the new simulation I would like to show off: http://rpubs.com/jjc/84238.
For those not familiar with my work on Bell, perhaps the best theoretical discussion to understand this simulation can be found here: http://arxiv.org/abs/1405.2355.
There is plenty of explanation in the preamble of the simulation itself, but the basic idea is to have sufficient structure of the 3-sphere (which is part of a well known solution of Einstein's field equations of general relativity) constructed in the preamble of the simulation before the actual correlations are computed. The locally explicable strong (or "quantum") correlations then follow from the structure of the 3-sphere itself, and the Bell-CHSH as well as CH inequalities are duly violated.
I don't think it is possible to improve on what I (with help) have produced in this simulation, but of course I would be delighted to be proven wrong about this.
Enjoy ,
Joy Christian
I have produced yet another simulation for the EPR-Bohm correlations which is more satisfactory and faithful to my 3-sphere model than previous attempts by myself and others. But before I describe it I want to thank Fred Diether, Michel Fodje, and Albert Jan Wonnink for ongoing discussions and help, as well as to some annoying, cynical, and persistent critics (such as Richard Gill) for keeping me on my toes about this.
So, without further ado, here is the new simulation I would like to show off: http://rpubs.com/jjc/84238.
For those not familiar with my work on Bell, perhaps the best theoretical discussion to understand this simulation can be found here: http://arxiv.org/abs/1405.2355.
There is plenty of explanation in the preamble of the simulation itself, but the basic idea is to have sufficient structure of the 3-sphere (which is part of a well known solution of Einstein's field equations of general relativity) constructed in the preamble of the simulation before the actual correlations are computed. The locally explicable strong (or "quantum") correlations then follow from the structure of the 3-sphere itself, and the Bell-CHSH as well as CH inequalities are duly violated.
I don't think it is possible to improve on what I (with help) have produced in this simulation, but of course I would be delighted to be proven wrong about this.
Enjoy ,
Joy Christian