过去一年中添加的文章,按日期排序
[HTML][HTML] Dark Energy predictions from GREA: Background and linear perturbation theory
J García-Bellido - Physics of the Dark Universe, 2024 - Elsevier
146 天前 - … horizon to the curvature scale, which provides a unique history of the Universe
distinguishable from that of Λ CDM. In particular, we explain the coincidence problem and the …
distinguishable from that of Λ CDM. In particular, we explain the coincidence problem and the …
Little ado about everything: ηCDM, a cosmological model with fluctuation-driven acceleration at late times
A Lapi, L Boco, MM Cueli, BS Haridasu… - The Astrophysical …, 2023 - iopscience.iop.org
355 天前 - … cosmic times without the need for any additional exotic component (eg, dark energy),
(ii) the spatial curvature … to show that the cosmic coincidence problem is relieved without …
(ii) the spatial curvature … to show that the cosmic coincidence problem is relieved without …
Dynamics of viable f(R) dark energy models in the presence of curvature–matter interactions
A Chatterjee, R Roy, S Dey… - The European Physical …, 2024 - Springer
356 天前 - … between dark matter and curvature-driven dark energy in … ) gravity models without
matter-curvature interactions as proposed … can also address the cosmic coincidence problem. …
matter-curvature interactions as proposed … can also address the cosmic coincidence problem. …
[HTML][HTML] Nonzero spatial curvature in symmetric teleparallel cosmology
A Paliathanasis - Physics of the Dark Universe, 2023 - Elsevier
357 天前 - … teleparallel theory to stand out are the new degree of freedom provided by the
connection defined in the non-coincidence frame which describes the nonzero spatial curvature. …
connection defined in the non-coincidence frame which describes the nonzero spatial curvature. …
相关搜索
- dark energy models
- asymptotically safe cosmology dark energy
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- effective dark energy
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- dynamical dark energy
- dark energy survey
- symmetric teleparallel cosmology nonzero spatial curvature
- scalar field models of dark energy
- observational constraints dark energy
- curvature matter sitter phase
- presence of curvature matter interactions
- curvature matter dynamical analysis