Induced Fission of Pu240 within a Real-Time Microscopic Framework
    
             Time-Dependent Superfluid Local Density Approximation
 
       Phys. Rev. Lett. 116, 122504 (2016),   DOI, pdf



Talks: 

      A. Bulgac, Tokyo, October 2015 (pdf, no videos)and with videos pptx
                        ECT*, Trento, Italy, June 8, 2016, pdf (17.9 MB, no videos) with videos pptx (255.8 MB)
                        INPC 2016, Adelaide, September 11-16, 2016, pptx(163.1 MB)
                        Fussion17, Hobart, Tasmania, 20-24 February, 2017, pptx
                        ECT*, Trento, Italy, March 20-25, 2017, pptx
      P. Magierski, GANIL, October 2015 (pdf, no videos)
      I. Stetcu, FUSTIPEN, March 2016,  pdf (no videos) or  pptx

If your default video player does not work, you can try VLC, which works for many video formats and several OS.
QuickTime will likely work well.

Videos:

Warning! Apparently the latest version of Firefox on macs with El Capitan has problems with opening the videos. The culprit appears to be Apple, who disabled the QuickTime plugin. In the Library/Internet Plug-Ins/Disabled Plug-Ins copy the two files in there and put them in the Internet Plug-Ins folder and restart Firefox and reactivate QuickTime at the prompt. Or, use another browser. I have tried Chrome, Safari, and SeaMonkey and they work.

A system of bearing balls rolling down, with and without obstacles. The obstacles simulate the presence of additional transversal degrees of freedom, which even though do not modify the value of the potential energy or of the mass, thus do not affect the speed, but change the length of the trajectory and thus of the time to reach destination. This is a simple realization of the Drude model for electron conduction.

Time evolution of the proton and neutron densities in S1-S3
Time evolution of the spatial amplitudes of the proton and neutron pairing field in S1-S3
Time evolution of the spatial amplitudes of the proton and neutron pairing fields in S1-S3 (slow)

Time evolution of the densities in S2 and S3
Time evolution of the densities in S2 and S3 (slow)
Time evolution of the pairing fields in S2 and S3
Time evolution of the pairing fields in S2 and S3 (slow)

Time evolution in S1
Time evolution in S1 (slow)

Time evolution in S2
Time evolution in S2 (slow)

Time evolution in S3

Time evolution in S4

Time evolution with currents S3
Time evolution with currents (slow) S3

Time evolution with currents (log scale) S3
Time evolution with currents (slow, log scale) S3