by Maxim Khlopov on Wed 23 May 2018 13:08
Dear Olga,
Thank you for draft. My comments are in the attached file.
General comment: use 'ordinary' not 'usual' and the term 'abundance of primordial helium'.
More essential: you should give more details of your physical model, specifying stable particles, which you predict in it as candidates for dark matter and possible mechanisms of inflation and baryosynthesis in it. If there are no such mechanisms, you should make assumption on your initial conditions: is temperature of ordinary and mirror matter equal in your scenario, do you assume equal baryon asymmetry in ordianry and mirror world and what is the role of your 4th mirror generation.
With the best regards
M.Yu.Khlopov
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[i]Хлопов Максим Юрьевич
Maxim Khlopov[/i]