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EuCAPT White Paper: Opportunities and Challenges for Theoretical Astroparticle Physics in the Next Decade

R. Alves Batista, +131 more
TLDR
The European Consortium for Astroparticle Theory (EuCAPT) white paper as mentioned in this paper explores upcoming theoretical opportunities and challenges for our field of research with particular emphasis on the possible synergies among different subfields, and the prospects for solving the most fundamental open questions with multi-messenger observations.
Abstract
Astroparticle physics is undergoing a profound transformation, due to a series of extraordinary new results, such as the discovery of high-energy cosmic neutrinos with IceCube, the direct detection of gravitational waves with LIGO and Virgo, and many others. This white paper is the result of a collaborative effort that involved hundreds of theoretical astroparticle physicists and cosmologists, under the coordination of the European Consortium for Astroparticle Theory (EuCAPT). Addressed to the whole astroparticle physics community, it explores upcoming theoretical opportunities and challenges for our field of research, with particular emphasis on the possible synergies among different subfields, and the prospects for solving the most fundamental open questions with multi-messenger observations.

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Citations
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Journal Article

The Observation of Gravitational Waves from a Binary Black Hole Merger

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Bow-Shock Pulsar Wind Nebulae Searches Aided by the North American Nanohertz Observatory for Gravitational Waves

TL;DR: The North American Nanohertz Observatory for Gravitational Waves (NANOW) is a collaboration of researchers who are actively engaged in using North American radio telescopes to detect and study gravitational waves (GWs) via pulsar timing.

Oscillons after Inflation

TL;DR: In this article, it was shown that in a class of well-motivated single-field models, inflation is followed by self resonance, leading to copious oscillon generation and a lengthy period of oscillon domination.

A Reverse Shock in GRB 130427A

TL;DR: In this paper, the authors present extensive radio and millimeter observations of the unusually bright GRB-130427A at z = 0.340, spanning 0.67-12 days after the burst.
Posted Content

A response to O. Arandjelovic's critique of "The reproducibility of research and the misinterpretation of p-values"

TL;DR: The main criticism of my piece in this article seems to be that my calculations rely on testing a point null hypothesis, i.e. the hypothesis that the true effect size is zero.
References
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Dark energy properties from large future galaxy surveys

TL;DR: In this paper, a detailed forecast on how well a Euclid-like survey will be able to constrain dark energy and neutrino parameters from a combination of its cosmic shear power spectrum, galaxy power spectrum and cluster mass function measurements was performed.
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Large-scale structure phenomenology of viable Horndeski theories

TL;DR: In this article, the authors studied the properties of π and π-Sigma functions in Horndeski theories with second order equations of motion and showed that they can be used to parameterize modifications of the growth of large-scale structure in alternative theories of gravity.
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Cosmological simulations of galaxy formation with cosmic rays

TL;DR: In this article, the authors investigate the dynamical impact of cosmic rays in cosmological simulations of galaxy formation using adaptive-mesh-based simulations of a 10 12 M ⊙ halo.
Journal ArticleDOI

Snowmass2021 - Letter of interest cosmology intertwined I: Perspectives for the next decade

Eleonora Di Valentino, +92 more
TL;DR: In this paper, the authors present a list of important goals that need to be addressed in the next decade, also taking into account the current discordances present between the different cosmological probes, as the Hubble constant H0 value, the σ8S8 tension, and the anomalies present in the Planck results.
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Probing Extreme-Density Matter with Gravitational Wave Observations of Binary Neutron Star Merger Remnants

TL;DR: In this article, the authors present a proof-of-concept study based on numerical-relativity simulations of how gravitational waves from neutron star merger remnants can probe the nature of matter at extreme densities.
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