Pseudoscalar Field as a Possible Candidate for Phantom Field

We demonstrate the existence of a single pseudoscalar (PS) field in the mathematically backed and parity‐preserving modifications of the standard Stückelberg formalism (SSF) in the context of the Lagrangian formulation of the (i) two (1 + 1)‐dimensional (2D) massive Abelian 1‐form gauge theory, (ii) three (2 + 1)‐dimensional (3D) massive Abelian 2‐form gauge theory, and (iii) four (3 + 1)‐dimensional (4D) massive Abelian 3‐form gauge theory. This PS field always turns up with the (i) negative kinetic term and (ii) higher order derivative terms. The latter terms are rendered into the well‐defined terms due to the imposition of the on‐shell condition for the PS field which is derived from the properly gauge‐fixed Lagrangian densities for the above theories. These Lagrangian densities incorporate into themselves the (i) PS field with the negative kinetic term and (ii) pure scalar field with the positive kinetic term. However, both these fields satisfy the Klein–Gordon (KG) equation of motion. The PS field (having the negative kinetic term and a well‐defined mass) is one of the possible candidates for the “phantom” field which plays a crucial role in the cyclic, bouncing, and self‐accelerated cosmological models of the universe. The “exotic” PS field also satisfies one of the criteria for being a possible candidate for dark matter.

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Publication Details

Journal
Advances in High Energy Physics
Published
2025-01-01
DOI
https://doi.org/10.1155/ahep/6687988
Citations
2
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
2.31

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article

Pseudoscalar Field as a Possible Candidate for Phantom Field

R. P. Malik, E. Harikumar
2 citations
Advances in High Energy Physics
Cosmology and Gravitation Theories
2.31
article

Pseudoscalar Field as a Possible Candidate for Phantom Field

R. P. Malik, E. Harikumar
article en
2 citations

Abstract

We demonstrate the existence of a single pseudoscalar (PS) field in the mathematically backed and parity‐preserving modifications of the standard Stückelberg formalism (SSF) in the context of the Lagrangian formulation of the (i) two (1 + 1)‐dimensional (2D) massive Abelian 1‐form gauge theory, (ii) three (2 + 1)‐dimensional (3D) massive Abelian 2‐form gauge theory, and (iii) four (3 + 1)‐dimensional (4D) massive Abelian 3‐form gauge theory. This PS field always turns up with the (i) negative kinetic term and (ii) higher order derivative terms. The latter terms are rendered into the well‐defined terms due to the imposition of the on‐shell condition for the PS field which is derived from the properly gauge‐fixed Lagrangian densities for the above theories. These Lagrangian densities incorporate into themselves the (i) PS field with the negative kinetic term and (ii) pure scalar field with the positive kinetic term. However, both these fields satisfy the Klein–Gordon (KG) equation of motion. The PS field (having the negative kinetic term and a well‐defined mass) is one of the possible candidates for the “phantom” field which plays a crucial role in the cyclic, bouncing, and self‐accelerated cosmological models of the universe. The “exotic” PS field also satisfies one of the criteria for being a possible candidate for dark matter.

Advances in High Energy PhysicsVol. 2025(1)
University of Hyderabad (IN), Banaras Hindu University (IN)
University of Hyderabad
Openalex Percentile: Top 12%
Cosmology and Gravitation Theories
2.31
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