Results 31 to 40 of about 3,462 (164)
We study the cosmological consequences of the extended uncertainty principle (EUP) by deriving modified Friedmann equations through thermodynamic arguments.
M. Roushan, N. Rashidi
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Dynamical Analysis of Scalar Field Cosmologies with Spatial Curvature
We explore the dynamical behaviour of cosmological models involving a scalar field (with an exponential potential and a canonical kinetic term) and a matter fluid with spatial curvature included in the equations of motion.
Mateja Gosenca, Peter Coles
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In this work, we studied four types of cosmological models with different mechanisms driving the accelerated expansion of the universe, include Braneworld models, Chaplygin Gas models, Emergent Dark Energy models, and cosmological torsion models ...
Ziqiang Liu +4 more
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The textbook N=1 supergravity has an F-term potential depending on a superpotential W (z i ) and a Kähler potential K z i z ¯ i ¯ $$ K\left({z}^i,{\overline{z}}^{\overline{i}}\right) $$ , with the scalar potential V z i z ¯ i ¯ $$ V\left({z}^i,{\overline{
Renata Kallosh, Andrei Linde
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Observações sobre as soluções clássicas da equação de Friedmann
As representações gráficas dos modelos clássicos de Friedmann frequentemente induzem ao erro, na discussão das idades dos universos-modelo. A maioria dos livros ignora as diferentes conceituais das representações no que diz respeito a estas idades ...
Arthur Viglioni, Domingos Soares
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It has recently been shown, in flat Robertson-Walker geometries, that the dynamics of gravitational actions which are minimally coupled to matter fields leads to the appearance of “attractors” - sets of physical observables on which phase space measures ...
David Sloan
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Quantum cosmological metroland model [PDF]
Relational particle mechanics is useful for modelling whole-universe issues such as quantum cosmology or the problem of time in quantum gravity, including some aspects outside the reach of comparably complex minisuperspace models. In this article, we consider the mechanics of pure shape and not scale of 4 particles on a line, so that the only ...
Anderson, E., Franzen, A.T.
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We test and compare coasting cosmological models with curvature parameters $k=\left\{-1,0,+1\right\}$ in ${H}_{0}^{2}{c}^{-2}$ units and the flat ΛCDM model by fitting them to cosmic chronometers (CCs), the Pantheon+ sample of Type Ia supernovae (SNe ...
Peter Raffai +4 more
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In this work, we study the applications of entropy bounds in two toy cosmological models with particle production (annihilation), i.e., a radiation-dominated universe and a dust-dominated universe.
Hao Yu, Jin Li
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Polynomial Affine Model of Gravity: After 10 Years
The polynomial affine model of gravity was proposed as an alternative to metric and metric-affine gravitational models. What, in the beginning, was thought to be a source of unpredictability—the presence of many terms in the action—turned out to be a ...
Oscar Castillo-Felisola +6 more
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