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A Review on the Scalar Field/ Bose-Einstein Condensate Dark Matter Model

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arxiv 1302.0903 v1 pith:KNXYK7EI submitted 2013-02-04 astro-ph.CO

Abril Suárez , Victor Robles , Tonatiuh Matos This is my paper · ORCID
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keywords modeldarkmatterbose-einsteincondensatefieldreviewscalar
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abstract

We review the work done so far aimed at modeling in an alternative way the dark matter in the Universe: the scalar field/ Bose-Einstein condensate dark matter (SFDM/BEC) model. We discuss a number of important achievements and characteristics of the model. We also describe some of our most recent results and predictions of the model compared to those of the standard model of $\Lambda$CDM.

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Forward citations

Cited by 7 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Core-Halo Mass Relation in Cosmological Vector Dark Matter

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    Confirmed Proca-star cores in vector dark matter follow M_star ≈ 2.65 M_halo^0.64, with only about 10% of halos hosting a detectable core.

  2. Tidal Love numbers of multi-state Boson stars

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    Quadrupolar electric tidal Love numbers of multi-state boson stars flip from positive to negative when mu~1 > 0.891 or omega~0 > 0.777, while magnetic Love numbers stay negative.

  3. Extreme mass-ratio inspirals into Newtonian Proca stars

    gr-qc 2026-07 accept novelty 6.0 of 10

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  4. Spin Polarization of Proca Stars Formed by Gravitational Bose--Einstein Condensation

    hep-ph 2026-07 unverdicted novelty 6.0 of 10

    Gravitationally condensed Proca stars exhibit partial spin polarization controlled by the elliptical polarization of the dominant component-space mode, with ensemble mean χ_net ≈ 0.62 and large realization-to-realizat...

  5. Nonrelativistic Proca stars: Spherical stationary and multi-frequency states

    gr-qc 2024-12 conditional novelty 6.0 of 10

    Nonrelativistic Proca stars have a ground state with constant polarization (linear or circular depending on the sign of the spin-spin coupling), and a symmetry-enhanced sector with λs=0 contains a continuum of multi-f...

  6. Quantum corrections as a Bound for Detecting Self-Interacting Ultralight Dark Matter

    hep-ph 2026-07 conditional novelty 5.0 of 10

    Radiative stability of the SIULDM potential under Yukawa couplings to SM fermions yields upper bounds on y that already intersect the projected reach of optical and nuclear clocks.

  7. Ultralight dark matter search in a large liquid scintillator detector

    hep-ph 2025-12 conditional novelty 5.0 of 10

    A JUNO-like detector could constrain the neutrino–ultralight-dark-matter oscillation-modulation parameters to ηΔ21 < 2.5×10^-2 and ηΔ31 < 5×10^-3 at 90% CL.

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