Cosmion-94: Proceedings of the First International Conference on CosmoParticle Physics Dedicated to the 80th Anniversary of YA B. Zeldovich and to the 5th Memorial of A.D. Sakharov |
Contents
A Rubakov | 11 |
A O Barvinsky A Yu Kamenshchik | 23 |
A A Kirillov V N Melnikov | 29 |
R Gavrilov V D Ivashchuk V N Melnikov | 35 |
A A Starobinsky | 43 |
K K Olkhin | 51 |
Yu A Kukharenko R F Polishchuk | 57 |
Yu Khlopov | 67 |
N Schramm C Copi | 77 |
S S Filippov M Yu Khlopov Yu L Levitan E V Sedelnikov I M Sobol | 93 |
Astrodamus collaboration | 99 |
P Chechev Ya M Kramarovsky O V Lozhkin | 113 |
K Enqvist A I Rez V B Semikoz | 119 |
Blinnikov I V Panov V M Chechetkin D A Ptitsin | 131 |
Common terms and phrases
abundance active allows amplitude analysis anisotropy assumed astrophysical background baryon calculations Center clusters component considered constant contribution corresponding cosmic cosmic rays cosmological dark matter decay density dependence detected determined direct discussed distribution effects electron elements emission energy equation estimate evolution existence experiments field Figure fluctuations flux formation frequency function fundamental galactic galaxy gamma-ray gives gravitational halo important increase inflation initial interactions Italy leads Lett light limit magnetic magnetic field mass mean measurements mechanism method monopole Moscow nature neutrino objects observed obtained parameters particles period perturbations photons Phys physical possible predicted present primordial problem processes produced radiation radio range rays References region relative Russian scale sensitivity separation shows simulations sources space spectra spectrum stage standard star string structure symmetry temperature theory Universe wave