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4741por Hahn, ChangHoon, Eickenberg, Michael, Ho, Shirley, Hou, Jiamin, Lemos, Pablo, Massara, Elena, Modi, Chirag, Moradinezhad Dizgah, Azadeh, Blancard, Bruno Régaldo-Saint, Abidi, Muntazir M.“…We present cosmological constraints from a simulation-based inference (SBI) analysis of galaxy clustering from the SimBIG forward modeling framework. …”
Publicado 2023
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4742“…We also discuss the unbiased determination of cosmological parameters from estimates of the power spectrum or experimental bandpowers.…”
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4743“…We do so using the boundary effective action formalism of hep-th/0401164 which accounts quantitatively for the cosmological vacuum ambiguity. In this formalism we can clearly 1) delineate the validity of cosmological effective actions in an expanding universe. …”
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4744“…We discuss the oscillations effects on neutrinos in the early Universe and update the cosmological constraints on the oscillation parameters. …”
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4745por Heywood, Paolo“…This article begins by examining the status of “difference” in representations of perspectivist cosmologies, which are themselves often represented as radically different to Euro-American cosmologies. …”
Publicado 2020
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4746“…The existence of minima with negative cosmological constant, stabilizing all moduli, is established. …”
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4747“…Dark energy models with a slowly rolling cosmological scalar field provide a popular alternative to the standard, time-independent cosmological constant model. …”
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4748“…Finally, we show that reliable nonperturbative calculations above the QCD crossover are needed to exploit the reach of upcoming cosmological surveys for axion detection.…”
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4749“…The central object of the method is the time-dependent probability distribution function generating correlators of the cosmological observables at a given moment of time. Expanding the distribution function around the Gaussian weight we formulate a perturbative technique to calculate non-linear corrections to cosmological correlators, similar to the diagrammatic expansion in a three-dimensional Euclidean quantum field theory, with time playing the role of an external parameter. …”
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4750por Floerchinger, Stefan“…Analytical results for relativistic scalar fields in cosmologies with 2+1 spacetime dimensions will be compared with recent experimental results obtained in Heidelberg laboratories.…”
Publicado 2023
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4751“…We study cosmological solutions in the context of 4-dimensional low energy Heterotic M-theory with moving bulk branes. …”
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4752“…This scenario satisfies terrestrial and cosmological constraints because it has neutrino self-interactions built-in. …”
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4753“…A curvature self-interaction of the cosmic gas is shown to mimic a cosmological constant or other forms of dark energy, such as a rolling tachyon condensate or a Chaplygin gas. …”
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4754“…In the context of a cosmological string model describing the propagation of strings in a time-dependent Robertson-Walker background space-time, we show that the asymptotic acceleration of the Universe can be identified with the square of the string coupling. …”
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4755
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4756“…Following a self-contained review of the basics of the theory of cosmological perturbations, we discuss why the conclusions reached in the recent paper by Kaloper et al are too pessimistic estimates of the amplitude of possible imprints of trans-Planckian (string) physics on the spectrum of cosmic microwave anisotropies in an inflationary Universe. …”
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4757por Laine, Mikko“…If there is a phase transition which is sufficiently strongly of the first order, important cosmological remnants could be produced, such as a baryon asymmetry. …”
Publicado 2001
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4758“…The proposed model provides a natural solution to the $\mu$-problem and is free from phenomenological and cosmological problems.…”
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4759por Lewandowski, Matthew“…As a main example, I will discuss our recent analysis of the BOSS galaxy-clustering power spectrum and bispectrum data using the one-loop predictions from the Effective Field Theory of Large-Scale Structure (EFTofLSS), where we find impressive constraints on cosmological parameters. Overall, we find that including higher-order predictions, which allows us to analyze the data to smaller length scales and access more physical modes, significantly reduces the error bars of cosmological parameters. …”
Publicado 2023
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4760por Lee, Hyun Min“…We consider the cosmological relaxation of the Higgs mass and the cosmological constant due to the four-form fluxes in four dimensions. …”
Publicado 2019
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