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On the recently proposed Mimetic Dark Matter

Published 10 Oct 2013 in gr-qc, astro-ph.CO, and hep-th | (1310.2790v2)

Abstract: Recently, an interesting gravitational model was proposed in order to mimic the effect of Dark Matter. Chamseddine and Mukhanov in the arXiv preprint 1308.5410 have separated the conformal mode of a physical metric in the form of a squared gradient of an auxiliary scalar field. Notably, the variational principle has given a more general equation of motion than that of purely Einsteinian relativity theory, with a possibility of reproducing an effective Dark Matter. In this short paper, we explain the nature of this phenomenon in terms of the class of functions on which the variation takes place. Then we give a more transparent equivalent formulation of the model without an auxiliary metric. Finally, we speculate a bit about possible extensions.

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Summary

Mimetic Dark Matter: A Novel Approach to Modifying Gravitational Interactions

The paper "On the Recently Proposed Mimetic Dark Matter" by Alexey Golovnev contributes to the ongoing discourse on alternative models of gravitational interaction designed to replicate the effects attributed to dark matter. Dark matter continues to be an enigmatic component of our universe, primarily detectable through its gravitational influences on cosmic structures. Despite extensive exploration, its true nature remains elusive. This paper delves into a novel gravitational model that circumvents conventional dark matter theory by modifying the variational principle underlying gravitational dynamics.

Overview and Formulation

Golovnev revisits the framework introduced by Chamseddine and Mukhanov, in which the standard metric in Einsteinian relativity is extended with contributions from an auxiliary metric and a scalar field of unusual dimension. This approach strategically disentangles the conformal mode from having any physical significance, transferring its role to the scalar field. The formulation reformulates the gravitational equations such that an auxiliary contribution mimics the pressureless dust typical of dark matter.

The model maintains consistency with Einstein's equations while introducing an effective stress tensor that represents mimetic dark matter. Gratifyingly, this formulation demands minimal departures from established gravitational models, thereby offering an elegant yet powerful tool in mimicking observed dark matter properties.

Key Contributions

The paper highlights notable distinctions in the model's formulation compared to traditional approaches by leveraging variational calculus. The enhanced freedom in the system results from derivative substitutions into the action without altering its fundamental components. Golovnev carefully reviews these modifications, especially the implications of the variational principle, to elucidate the genesis of extra contributions which resemble dark matter.

Golovnev proposes an equivalent formulation comprising Lagrange multipliers, optimizing the constraint fixing term within the action. This formulation accomplishes model equivalency while harnessing the scalar field to mimic dark matter behavior through simplified mathematical constructs.

Implications and Future Directions

This mimetic dark matter model signifies an intriguing avenue that might explain dark matter phenomena purely through the modification of gravitational principles, devoid of actual dark matter particles. Such theoretical constructs offer exciting possibilities for reconciling discrepancies between observable phenomena and standard cosmological models.

Further speculations in the paper about extending this model involve promoting the Lagrange multiplier to a physical field under specific conditions. Golovnev suggests introducing a kinetic term and potential to the Lagrange multiplier, which might offer insight into more complex gravitational scenarios.

Golovnev's analysis paves the path for future research, aiming at incorporating these mimetic frameworks into broader cosmological models and potential phenomenological applications. This might result in significant advancements in theoretical physics, particularly in understanding the universe's dark sector.

In conclusion, the exploration of mimetic dark matter models reiterates the potential richness of gravitational model building in cosmology. Continued investigations into these theoretical frameworks might ultimately illuminate further aspects of dark matter and contribute to a more comprehensive understanding of cosmic structure.

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