Felder, Gary; Tkachev, Igor LATTICEEASY: A program for lattice simulations of scalar fields in an expanding universe. (English) Zbl 1196.83005 Comput. Phys. Commun. 178, No. 12, 929-932 (2008). Summary: We describe a C++ program that we have written and made available for calculating the evolution of interacting scalar fields in an expanding universe. The program is particularly useful for the study of reheating and thermalization after inflation. The program and its full documentation are available on the Web at http://www.science.smith.edu/departments/Physics/fstaff/gfelder/latticeeasy/. In this paper we provide a brief overview of what the program does and what it is useful for. Cited in 31 Documents MSC: 83-04 Software, source code, etc. for problems pertaining to relativity and gravitational theory Keywords:LATTICEEASY; inflation; reheating; lattice simulations; classical field theory Software:LATTICEEASY PDFBibTeX XMLCite \textit{G. Felder} and \textit{I. Tkachev}, Comput. Phys. Commun. 178, No. 12, 929--932 (2008; Zbl 1196.83005) Full Text: DOI arXiv References: [1] A.D. Linde, Particle Physics and Inflationary Cosmology, Harwood, Chur, Switzerland, 1990; A.D. Linde, Particle Physics and Inflationary Cosmology, Harwood, Chur, Switzerland, 1990 [2] Khlebnikov, S.; Tkachev, I., Phys. Rev. Lett., 77, 219 (1996) [3] Khlebnikov, S.; Tkachev, I., Phys. Rev. Lett., 79, 1607 (1997) [4] Khlebnikov, S.; Tkachev, I., Phys. Rev. D, 56, 653 (1997) [5] Kofman, L.; Linde, A.; Starobinsky, A. A., Phys. Rev. D, 56, 3258 (1997) [6] Kolb, E. W.; Riotto, A.; Tkachev, I., Phys. Lett. B, 423, 348 (1998) [7] Khlebnikov, S.; Kofman, L.; Linde, A.; Tkachev, I., Phys. Rev. Lett., 81, 2012 (1998) [8] Tkachev, I.; Khlebnikov, S.; Kofman, L.; Linde, A., Phys. Lett. B, 440, 262 (1998) [9] Felder, G.; Kofman, L.; Linde, A.; Tkachev, I., JHEP, 0008, 010 (2000) [10] Kolb, E. W.; Riotto, A.; Tkachev, I., Phys. Rev. D, 56, 6133 (1997) [11] Polarski, D.; Starobinsky, A., Class. Quant. Grav., 13, 377 (1996) This reference list is based on information provided by the publisher or from digital mathematics libraries. Its items are heuristically matched to zbMATH identifiers and may contain data conversion errors. In some cases that data have been complemented/enhanced by data from zbMATH Open. This attempts to reflect the references listed in the original paper as accurately as possible without claiming completeness or a perfect matching.