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Euclid. I. Overview of the Euclid mission
/ Euclid Collaboration
The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. [...]
arXiv:2405.13491.
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94.
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Gravitational probes of ultra-light axions
/ Grin, Daniel (Haverford Coll.) ; Amin, Mustafa A. (Rice U.) ; Gluscevic, Vera (Florida U. ; Princeton U.) ; Grin, Daniel (Haverford Coll.) ; Hlǒzek, Renée (Toronto U., Astron. Dept.) ; Marsh, David J.E. (Inst. Astrophys. Gottingen) ; Poulin, Vivian (U. Montpellier 2, LUPM ; Johns Hopkins U.) ; Prescod-Weinstein, Chanda (New Hampshire U.) ; Smith, Tristan L. (Swarthmore Coll.) ; Ahmed, Zeeshan (SLAC) et al.
The axion is a hypothetical, well-motivated dark-matter particle whose existence would explain the lack of charge-parity violation in the strong interaction. [...]
arXiv:1904.09003.
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17 p.
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Synergy between cosmological and laboratory searches in neutrino physics
/ Gerbino, Martina (UC, Irvine ; INFN, Ferrara) ; Grohs, Evan (Victoria U. ; North Carolina State U.) ; Lattanzi, Massimiliano (Ferrara U. ; INFN, Ferrara) ; Abazajian, Kevork N. (UC, Irvine) ; Blinov, Nikita (Victoria U.) ; Brinckmann, Thejs (Ferrara U. ; INFN, Ferrara) ; Chen, Mu-Chun (UC, Irvine) ; Djurcic, Zelimir (Argonne) ; Du, Peizhi (YITP, Stony Brook) ; Escudero, Miguel (Munich, Tech. U.) et al.
The intersection of the cosmic and neutrino frontiers is a rich field where much discovery space still remains. Neutrinos play a pivotal role in the hot big bang cosmology, influencing the dynamics of the universe over numerous decades in cosmological history. [...]
arXiv:2203.07377; FERMILAB-PUB-22-207-V.-
2023-09-22 - 56 p.
- Published in : Phys. Dark Univ.: 42 (2023) , pp. 101333
Fulltext: 1f639c52895e4c52794b8f4474b183b7 - PDF; 2203.07377 - PDF; FERMILAB-PUB-22-207-V - PDF; External links: Fermilab Accepted Manuscript; eConf
In : 2021 Snowmass Summer Study, Seattle, WA, United States, 11 - 20 July 2021, pp.101333
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Neutrino Self-Interactions: A White Paper
/ Berryman, Jeffrey M. (Washington U., Seattle ; UC, Berkeley) ; Blinov, Nikita (Victoria U.) ; Brdar, Vedran (Fermilab ; Northwestern U.) ; Brinckmann, Thejs (INFN, Ferrara ; Ferrara U.) ; Bustamante, Mauricio (Bohr Inst.) ; Cyr-Racine, Francis-Yan (New Mexico U.) ; Das, Anirban (SLAC) ; de Gouvêa, André (Northwestern U.) ; Denton, Peter B. (Brookhaven Natl. Lab.) ; Dev, P.S. Bhupal (Washington U., St. Louis) et al.
Neutrinos are the Standard Model (SM) particles which we understand the least, often due to how weakly they interact with the other SM particles. Beyond this, very little is known about interactions among the neutrinos, i.e., their self-interactions. [...]
arXiv:2203.01955; CERN-TH-2022-024; DESY-22-035; FERMILAB-PUB-22-099-T.-
2023-06-09 - 39 p.
- Published in : Phys. Dark Univ.: 42 (2023) , pp. 101267
Fulltext: jt - PDF; 2203.01955 - PDF; External links: Fermilab Library Server; eConf
In : 2021 Snowmass Summer Study, Seattle, WA, United States, 11 - 20 July 2021, pp.101267
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CMB-S4: Forecasting Constraints on Primordial Gravitational Waves
/ CMB-S4 Collaboration
CMB-S4---the next-generation ground-based cosmic microwave background (CMB) experiment---is set to significantly advance the sensitivity of CMB measurements and enhance our understanding of the origin and evolution of the Universe, from the highest energies at the dawn of time through the growth of structure to the present day. [...]
arXiv:2008.12619 ; FERMILAB-PUB-20-468-AE-SCD.
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24 p.
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Dark Matter Science in the Era of LSST
/ Bechtol, Keith (Wisconsin U., Madison) ; Drlica-Wagner, Alex (Chicago U., Astron. Astrophys. Ctr. ; Chicago U., KICP ; Fermilab) ; Abazajian, Kevork N. (UC, Irvine) ; Abidi, Muntazir (Cambridge U., DAMTP) ; Adhikari, Susmita (KIPAC, Menlo Park) ; Ali-Haïmoud, Yacine (New York U.) ; Annis, James (Fermilab) ; Ansarinejad, Behzad (Durham U.) ; Armstrong, Robert (LLNL, Livermore) ; Asorey, Jacobo (Queensland U. ; Unlisted, AU) et al.
Astrophysical observations currently provide the only robust, empirical measurements of dark matter. [...]
arXiv:1903.04425.
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2019. - 11 p.
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Planck 2018 results. I. Overview and the cosmological legacy of Planck
/ Planck Collaboration
The European Space Agency's Planck satellite, which was dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013, producing deep, high-resolution, all-sky maps in nine frequency bands from 30 to 857GHz. [...]
arXiv:1807.06205.-
2020-09-01 - 56 p.
- Published in : Astron. Astrophys. 641 (2020) A1
Fulltext: 1807.06205 - PDF; arXiv:1807.06205 - PDF;
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Exploring cosmic origins with CORE: Survey requirements and mission design
/ CORE Collaboration
Future observations of cosmic microwave background (CMB) polarisation have the potential to answer some of the most fundamental questions of modern physics and cosmology. In this paper, we list the requirements for a future CMB polarisation survey addressing these scientific objectives, and discuss the design drivers of the CORE space mission proposed to ESA in answer to the "M5" call for a medium-sized mission. [...]
arXiv:1706.04516.-
2018-04-05 - 79 p.
- Published in : JCAP
Fulltext: PDF; Preprint: PDF;
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Exploring Cosmic Origins with CORE: Inflation
/ Finelli, Fabio (Bologna Observ. ; INFN, Bologna) ; Bucher, Martin (APC, Paris) ; Achúcarro, Ana (Leiden U. ; Basque U., Bilbao) ; Ballardini, Mario (Bologna U. ; Bologna Observ. ; INFN, Bologna) ; Bartolo, Nicola (Padua U. ; INFN, Padua ; Padua Observ.) ; Baumann, Daniel (Cambridge U., DAMTP ; Amsterdam U.) ; Clesse, Sébastien (Aachen, Tech. Hochsch.) ; Errard, Josquin (ILP, Paris ; Paris U., VI-VII) ; Handley, Will (Cambridge U. ; Cambridge U., KICC) ; Hindmarsh, Mark (Sussex U. ; Helsinki Inst. of Phys. ; Helsinki U.) et al.
/CORE
We forecast the scientific capabilities to improve our understanding of cosmic inflation of CORE, a proposed CMB space satellite submitted in response to the ESA fifth call for a medium-size mission opportunity. The CORE satellite will map the CMB anisotropies in temperature and polarization in 19 frequency channels spanning the range 60-600 GHz. [...]
arXiv:1612.08270.-
2018-04-05 - 100 p.
- Published in : JCAP 04 (2018) 016
Fulltext: PDF;
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