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Source: paper_references, paper_reference_links, observed 2026-08-11T18:20:41.538111Z
Paper Citation Record · LEDGER
As of 12 August 2026, this Paper Citation Record lists 96 of 96 outbound references and 0 inbound Pith citation observations for arXiv:2608.09390.
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Source: paper_references, paper_reference_links, observed 2026-08-11T18:20:41.538111Z
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96 of 96 outbound references displayed
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Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology Cluster counts III. $\Lambda$CDM extensions and the cluster tension
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Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology $\Lambda_{\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions
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Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology (29) For a radiation-dominated universe ( ω = 1 /3), the con- tinuity equation gives ρ = ρ0a−4, leading to the scale factor evolution a(t) ∼ t1/2 (since H = ˙a/a ∼ t−1/2)
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Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology Analysis of the Yukawa gravitational potential in $f(R)$ gravity I: semiclassical periastron advance
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Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology Differentiating with respect to time and using ˙H = dH/dt, for a flat universe ( k = 0) we obtain ˙H ( 1 − α 2λ2(1 + α) H −2 ) = − 4πG 1 + α (ρ + p)
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Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology where C = H 2 GR/(1 + α) and ǫ = Γ ln H 2
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Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology Observations of primordial 4He, assuming η10 = 6, give Yp = 0 .2449 ± 0.004 [ 22]
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Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology Archidiacono, E
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Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology An Introduction to Particle Dark Matter
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Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology Precise Relic WIMP Abundance and its Impact on Searches for Dark Matter Annihilation
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Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology A Modified Scalar-Tensor-Vector Gravity Theory and the Constraint on its Parameters
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Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology (92) It is convenient to rewrite the above equation in the form ds(T ) dt = −3Hs(T ) → dt = − ds(T ) 3s(T ) H −1
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Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology Constraining the range of Yukawa gravity interaction from S2 star orbits
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Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology Constraints on Yukawa gravity parameters from observations of bright stars
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Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology Scalar field effects on the orbit of S2 star
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Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology Testing Yukawa cosmology at the Milky Way and M31 galactic scales
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Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology Weinberg, Cosmology, New York: Oxford University press, (2008)
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