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Inflation and late-time cosmic acceleration in non-minimal Maxwell-$F(R)$ gravity and the generation of large-scale magnetic fields

Published 7 Jan 2008 in gr-qc, hep-ph, and hep-th | (0801.0954v2)

Abstract: We study inflation and late-time acceleration in the expansion of the universe in non-minimal electromagnetism, in which the electromagnetic field couples to the scalar curvature function. It is shown that power-law inflation can be realized due to the non-minimal gravitational coupling of the electromagnetic field, and that large-scale magnetic fields can be generated due to the breaking of the conformal invariance of the electromagnetic field through its non-minimal gravitational coupling. Furthermore, it is demonstrated that both inflation and the late-time acceleration of the universe can be realized in a modified Maxwell-$F(R)$ gravity which is consistent with solar system tests and cosmological bounds and free of instabilities. At small curvature typical for current universe the standard Maxwell theory is recovered. We also consider classically equivalent form of non-minimal Maxwell-$F(R)$ gravity, and propose the origin of the non-minimal gravitational coupling function based on renormalization-group considerations.

Citations (214)

Summary

  • The paper demonstrates a non-minimal coupling of the electromagnetic field with scalar curvature R to break conformal invariance and generate quantum fluctuations during inflation.
  • It shows that power-law inflation and late-time cosmic acceleration can be realized within Maxwell-F(R) gravity, aligning with observational tests and solar-system constraints.
  • The research indicates that energy density from generated large-scale magnetic fields may substantially influence cosmic evolution and unify early and late universe dynamics.

Overview of Non-Minimal Maxwell-F(R) Gravity and its Cosmological Implications

The paper by Kazuharu Bamba and Sergei D. Odintsov addresses a prominent issue in cosmology, namely, the dynamics of inflation and late-time cosmic acceleration within a modified gravity framework. Specifically, it investigates the role of non-minimal electromagnetic interactions in Maxwell-F(R) gravity and their capability to generate large-scale magnetic fields. This research presents a modified approach to understanding inflation and dark energy that does not solely rely on classical explanations involving dark matter and dark energy but considers the broader impacts of coupling gravitational and electromagnetic fields.

Key Contributions

The paper presents several key contributions to the field:

  1. Non-Minimal Electromagnetic Coupling: The authors propose a model where the electromagnetic field is non-minimally coupled to the scalar curvature R. This framework breaks the standard conformal invariance, facilitating the generation of electromagnetic quantum fluctuations. These fluctuations are proposed as significant contributors to the inflationary phase of the universe and could manifest as observable large-scale magnetic fields.
  2. Inflation and Cosmic Acceleration: The study demonstrates the feasibility of realizing both inflation and the late-time acceleration of the universe with modified Maxwell-F(R) gravity, which remains consistent with current cosmological observations and solar-system tests without leading to instabilities. This is achieved through a classically equivalent form of this gravity theory, implying a unification scheme for the cosmic inflation and acceleration phenomena.
  3. Renormalization Group Considerations: The origin of non-minimal gravitational coupling is explored while discussing renormalization group implications. This approach potentially connects the modifications at high energy scales to quantum corrections observed at different stages of the universe's evolution.

Numerical Findings and Theoretical Implications

The results highlight the power-law inflation induced by the non-minimal gravitational coupling to electromagnetic fields. The paper also suggests that the energy density of the large-scale magnetic fields generated during inflation could play a pivotal role in cosmic evolution, thereby providing a robust mechanism for extending standard F(R) gravity frameworks.

The functional forms of both F(R) and the electromagnetic coupling I(R) suggest that these elements could behave effectively as cosmological constants under certain limits, presenting a new perspective on the unification of early universe physics and late-time cosmic dynamics.

Future Prospects and Observational Tests

Future theoretical advancements and observational endeavors could confirm the presence of large-scale magnetic fields, which, if corroborated, would imply the necessity of modifying existing gravitational theories to include electromagnetic couplings. Such a detection would further necessitate refining the parameters of the proposed model to align predictions with empirical data.

In conclusion, the paper provides an incisive analysis of how incorporating non-minimal electromagnetic interactions in modified gravity theories might answer unresolved questions about cosmic inflation and the accelerated expansion of the universe. It challenges conventional paradigms by proposing an integrated framework that can be tested against future experimental data, potentially broadening the scope of cosmological models and providing novel insights into the unification of forces at cosmic scales.

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