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This article is cited in 16 scientific papers (total in 16 papers)
Total energy potential as a superpotential in integrable cosmological models
A. V. Yurova, V. A. Yurovab, S. V. Chervonc, M. Samid a Immanuel Kant State University of Russia, Kaliningrad,
Russia
b Department of Mathematics, University of Missouri, Columbia,
Missouri, USA
c Ul'yanovsk State Pedagogical University, Ul'yanovsk, Russia
d Centre for Theoretical Physics, Jamia Millia Islamia
(A Central University), New Delhi, India
Abstract:
We study the class of integrable self-action potentials satisfying the conditions that (1) they spontaneously break the symmetry, (2) they describe the inflation phase with a graceful exit (i.e., with an exit that does not require fine tuning parameters), and (3) they feature several consecutive inflation phases. The first condition ensures that the inflation mechanism is qualitatively consistent with elementary particle physics, the second is a necessary ingredient of any inflation theory, and the third is necessary for a theory to be consistent with contemporary observational data, which support the accelerated expansion of the Universe.
Keywords:
superpotential, inflation, Friedmann equations.
Received: 15.05.2010 Revised: 18.08.2010
Citation:
A. V. Yurov, V. A. Yurov, S. V. Chervon, M. Sami, “Total energy potential as a superpotential in integrable cosmological models”, TMF, 166:2 (2011), 299–311; Theoret. and Math. Phys., 166:2 (2011), 259–269
Linking options:
https://www.mathnet.ru/eng/tmf6611https://doi.org/10.4213/tmf6611 https://www.mathnet.ru/eng/tmf/v166/i2/p299
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Abstract page: | 633 | Full-text PDF : | 257 | References: | 68 | First page: | 26 |
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