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1.
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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.
Fulltext
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2.
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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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3.
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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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4.
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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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5.
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The Polarized Radiation Imaging and Spectroscopy Mission
/ PRISM Collaboration
PRISM (Polarized Radiation Imaging and Spectroscopy Mission) was proposed to ESA in May 2013 as a large-class mission for investigating within the framework of the ESA Cosmic Vision program a set of important scientific questions that require high resolution, high sensitivity, full-sky observations of the sky emission at wavelengths ranging from millimeter-wave to the far-infrared. PRISM's main objective is to explore the distant universe, probing cosmic history from very early times until now as well as the structures, distribution of matter, and velocity flows throughout our Hubble volume [...]
arXiv:1310.1554.-
2014-02-05 - 55 p.
- Published in : JCAP 02 (2014) 006
Fulltext: PDF; External link: Preprint
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6.
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Cosmological lepton asymmetry with a nonzero mixing angle $\theta_{13}$
/ Castorina, Emanuele (SISSA, Trieste) ; Franca, Urbano (Valencia U., IFIC) ; Lattanzi, Massimiliano (Milan Bicocca U.) ; Lesgourgues, Julien (CERN ; IPT, Lausanne ; Annecy, LAPTH) ; Mangano, Gianpiero (INFN, Naples) ; Melchiorri, Alessandro (Rome U.) ; Pastor, Sergio (Valencia U., IFIC)
While the baryon asymmetry of the Universe is nowadays well measured by cosmological observations, the bounds on the lepton asymmetry in the form of neutrinos are still significantly weaker. We place limits on the relic neutrino asymmetries using some of the latest cosmological data, taking into account the effect of flavor oscillations. [...]
arXiv:1204.2510; CERN-PH-TH-2012-089; IFIC-12-28; LAPTH-018-12.-
2012
- Published in : Phys. Rev. D 86 (2012) 023517
APS Published version, local copy: PDF; External link: Preprint
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7.
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Model independent constraints on mass-varying neutrino scenarios
/ Franca, Urbano (Valencia U., IFIC) ; Lattanzi, Massimiliano (Rome U.) ; Lesgourgues, Julien (CERN ; Annecy, LAPTH) ; Pastor, Sergio (Valencia U., IFIC)
Models of dark energy in which neutrinos interact with the scalar field supposed to be responsible for the acceleration of the universe usually imply a variation of the neutrino masses on cosmological time scales. In this work we propose a parameterization for the neutrino mass variation that captures the essentials of those scenarios and allows to constrain them in a model independent way, that is, without resorting to any particular scalar field model. [...]
arXiv:0908.0534; CERN-PH-TH-2009-144.-
2009 - 13 p.
- Published in : Phys. Rev. D 80 (2009) 083506
APS Published version, local copy: PDF; Fulltext: PDF; External link: Preprint
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