Initialized the project.
Change viscous correction to new conventions.
clean up
Solving the issue 1
Modified to pi^{\mu\nu} \hat{q}_\mu \hat_\nu, still need to be debugged.
Fixed the bug caused by changing the order of for loop for q and q_phi
Almost there... Fixed lorentz contraction for pi^munu tensor with q_mu q_nu. Tested the results against previous results from boost and rotation and they agree with each other.
Change the filenames of rates to be the same as the output from the rate calculation codes.
Change the filename of the rates to be consistent
Add sin terms for v_n flow and some clean up
issue 4 is resolved, and the code has passed a simple check test. I changed the parameters file to be consistent with s95p-v0-PCE
Add EOS class to handle interpolation between varies thermaldynamic quantities. Add error function in Arsenal to output error message from functions.
use better function name in EOS class, do not need to keep track on column number
Fixed some bugs in EOS.cpp and add Bjorken scaling for energy density and pressure which are used in the calculations of viscous corrections.
some clean ups ..
Clean up the setups for read in photon emission rates in the initialization stage.
Merge branch 'iss3'
I resolved issue 3 about the limitation of the EOS table for initial 1D Bjorken back trace procedure.
Begin to solve issue 2. Hydro info are now read from hdf5 files.
passed compile stage...
Add flag to decide whether to calculate HG individual channels. I put loop for time frame into photonemission class. Bjorken expansion needs further modifications. Functions to calculate total hadronic photons in Photonemssion needs to clean out. Whole simulations needs to be tested against previous results.