15 Wilczek F, “Reheating An Inflationary Universe,” Phys. Rev. Lett. 48 , 1437 (1982). [4] Traschen JH, Brandenberger RH “Particle Production During Out-Of-Equilibrium Phase Transitions,” Phys. Rev. D 42 , 2491 (1990). [5] Dolgov AD, Kirilova DP, “Production of particles by a variable scalar field,” Sov. J. Nucl. Phys. 51 , 172 (1990) [Yad. Fiz. 51 , 273 (1990)]. [6] Boyanovsky D, de Vega HJ, R. Holman R, “Nonequilib- rium evolution of scalar fields in FRW cosmologies I,” Phys. Rev. D 49 , 2769 (1994); Boyanovsky D, de Vega HJ, Holman R, Lee DS, Singh A, “Dissipation Via Par- ticle Production In Scalar Field Theories,” Phys. Rev. D 51 , 4419 (1995); Boyanovsky D, D’Attanasio MD, de Vega HJ, Holman R, Lee DS, “Reheating and thermal- ization: Linear versus nonlinear relaxation,” Phys. Rev. D 52 , 6805 (1995); Boyanovsky D, de Vega HJ, Hol- man R, Salgado JFJ, “Analytic and numerical study of preheating dynamics,” Phys. Rev. D 54 , 7570 (1996); Boyanovsky D, Cormier D, de Vega HJ, Holman R, Singh A, Srednicki M, “Scalar field dynamics in Fried- man Robertson Walker spacetimes,” Phys. Rev. D 56 , 1939 (1997); Cormier D, Heitmann K, Mazumdar A, “Dynamics of coupled bosonic systems with applications to preheating,” Phys. Rev. D 65 , 083521 (2002). [7] Baacke J, Heitmann K, C. Patzold C, “Nonequilibrium dynamics: A renormalized computation scheme,” Phys. Rev. D 55 , 2320 (1997); Baacke J, Heitmann K, Patzold C, “Nonequilibrium dynamics: Preheating in the SU(2) Higgs model,” Phys. Rev. D 55 , 7815 (1997). Baacke J, Heitmann K, Patzold C, “On the choice of initial states in nonequilibrium dynamics,” Phys. Rev. D 57 , 6398 (1998). [8] Kofman L, Linde AD, Starobinsky AA, “Reheating after inflation,” Phys. Rev. Lett. 73 , 3195 (1994). [9] Shtanov Y, Traschen JH, Brandenberger RH, “Universe reheating after inflation,” Phys. Rev. D 51 , 5438 (1995); Shtanov, Y., Ukr. Fiz. Zh. 38 , 1425 (1993). [10] Kofman L, Linde AD, Starobinsky AA, “Towards the theory of reheating after inflation,” Phys. Rev. D 56 , 3258 (1997). [11] Micha R, Tkachev II, “Relativistic turbulence: A long way from preheating to equilibrium,” Phys. Rev. Lett. 90 , 121301 (2003); Micha R, Tkachev II, “Turbulent thermalization,” Phys. Rev. D 70 , 043538 (2004). [12] Brandenberger RH, “Quantum Field Theory Methods And Inflationary Universe Models,” Rev. Mod. Phys. 57 , 1 (1985). [13] Bezrukov FL, Shaposhnikov M, “The SM Higgs boson as the inflaton,” Phys. Lett. B 659 , 703 (2008). [14] Linde AD, “A New Inflationary Universe Scenario: A Possible Solution Of The Horizon, Flatness, Homo- geneity, Isotropy And Primordial Monopole Problems,” Phys. Lett. B 108 , 389 (1982). [15] Albrecht AJ, Steinhardt PJ, “Cosmology For Grand Unified Theories With Radiatively Induced Symmetry Breaking,” Phys. Rev. Lett. 48 , 1220 (1982). [16] Coleman SR, Weinberg EJ, “Radiative Corrections As The Origin Of Spontaneous Symmetry Breaking,” Phys. Rev. D 7 , 1888 (1973). [17] Goldwirth DS, Piran T, “Initial conditions for infla- tion,” Phys. Rept. 214 , 223 (1992); Albrecht AJ, Bran- denberger RH, “On The Realization Of New Inflation,” Phys. Rev. D 31 , 1225 (1985). [18] Linde AD, “Chaotic Inflation,” Phys. Lett. B 129 , 177 (1983). [19] Brandenberger RH, Kung JH, “Chaotic Inflation As An Attractor In Initial Condition Space,” Phys. Rev. D 42 , 1008 (1990). [20] Feldman HA, Brandenberger RH, “Chaotic Inflation With Metric And Matter Perturbations,” Phys. Lett. B 227 , 359 (1989). [21] Linde AD, “Hybrid inflation,” Phys. Rev. D 49 , 748 (1994). [22] Gleiser M, Ramos RO, “Microphysical approach to nonequilibrium dynamics of quantum fields,” Phys. Rev. D 50 , 2441 (1994). [23] Kaiser DI, “Preheating in an expanding universe: Ana- lytic results for the massless case,” Phys. Rev. D 56 , 706 (1997); Kaiser DI, “Resonance structure for preheating with massless fields,” Phys. Rev. D 57 , 702 (1998). [24] Greene PB, Kofman L, Linde AD, Starobinsky AA, “Structure of resonance in preheating after inflation,” Phys. Rev. D 56 , 6175 (1997). [25] Greene PB, Kofman L, Starobinsky AA, “Sine-Gordon parametric resonance,” Nucl. Phys. B 543 , 423 (1999). [26] Birrell ND, Davies PCW, “Quantum Fields In Curved Space,” Cambridge, Uk: Univ. Pr. ( 1982) 340p [27] McLachlan NW, “Theory and Applications of Mathieu Functions” (Oxford Univ. Press, Clarendon, 1947). [28] Greene PB, Kofman L, “Preheating of fermions,” Phys. Lett. B 448 , 6 (1999); Greene PB, Kofman L, “On the theory of fermionic preheating,” Phys. Rev. D 62 , 123516 (2000). [29] Baacke J, Heitmann K, Patzold C, “Nonequilibrium dy- namics of fermions in a spatially homogeneous scalar background field,” Phys. Rev. D 58 , 125013 (1998). [30] Cyr-Racine F-Y, McGill Univ. MSc thesis, 2008 (un- published). [31] Khlebnikov SY, Tkachev II, “Classical decay of infla- ton,” Phys. Rev. Lett. 77 , 219 (1996). [32] Khlebnikov SY, Tkachev II, “The universe after infla- tion: The wide resonance case,” Phys. Lett. B 390 , 80 (1997). [33] Khlebnikov SY, Tkachev II, “Resonant decay of Bose condensates,” Phys. Rev. Lett. 79 , 1607 (1997). [34] Prokopec T, Roos TG, “Lattice study of classical infla- ton decay,” Phys. Rev. D 55 , 3768 (1997). [35] Greene BR, Prokopec T, Roos TG, “Inflaton decay and heavy particle production with negative coupling,” Phys. Rev. D 56 , 6484 (1997). [36] Shuhmaher N, Brandenberger RH, “Non-perturbative instabilities as a solution of the cosmological moduli problem,” Phys. Rev. D 73 , 043519 (2006). [37] Dufaux J-F, Felder GN, Kofman L, Peloso M, Podolsky D, “Preheating with Trilinear Interactions: Tachyonic Resonance,” JCAP 0607 , 006 (2006). [38] Abolhasani AA, Firouzjahi H, Sheikh-Jabbari MM, “Tachyonic Resonance Preheating in Expanding Uni- verse,” arXiv:0912.1021 [hep-th]. [39] Felder GN, Garcia-Bellido J, Greene PB, Kofman L, Linde AD, Tkachev I, “Dynamics of symmetry breaking and tachyonic preheating,” Phys. Rev. Lett. 87 , 011601 (2001). [40] Felder GN, Kofman L, Linde AD, “Tachyonic instabil- ity and dynamics of spontaneous symmetry breaking,” Phys. Rev. D 64 , 123517 (2001). [41] Garcia-Bellido J, Linde AD, “Preheating in hybrid in-