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CERN Document Server 13 Datensätze gefunden  1 - 10nächste  gehen zum Datensatz: Die Suche hat 0.60 Sekunden gedauert. 
1.
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. - 94.
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2.
Euclid. IV. The NISP Calibration Unit / Euclid Collaboration
The near-infrared calibration unit (NI-CU) on board Euclid's Near-Infrared Spectrometer and Photometer (NISP) is the first astronomical calibration lamp based on light-emitting diodes (LEDs) to be operated in space. [...]
arXiv:2405.13494. - 21.
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3.
Euclid: Constraining linearly scale-independent modifications of gravity with the spectroscopic and photometric primary probes / Euclid Collaboration
The future Euclid space satellite mission will offer an invaluable opportunity to constrain modifications to Einstein's general relativity at cosmic scales. We focus on modified gravity models characterised, at linear scales, by a scale-independent growth of perturbations while featuring different testable types of derivative screening mechanisms at smaller non-linear scales [...]
arXiv:2306.12368.- 2024-10-01 - 22 p. - Published in : Astron. Astrophys. 690 (2024) A133 Fulltext: 2306.12368 - PDF; Publication - PDF; document - PDF;
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4.
EuCAPT White Paper: Opportunities and Challenges for Theoretical Astroparticle Physics in the Next Decade / Alves Batista, R. (Madrid, IFT) ; Amin, M.A. (Rice U.) ; Barenboim, G. (Valencia U.) ; Bartolo, N. (U. Padua, Dept. Phys. Astron.) ; Baumann, D. (Amsterdam U. ; U. Amsterdam, GRAPPA ; U. Edinburgh, Higgs Ctr. Theor. Phys.) ; Bauswein, A. (Darmstadt, GSI) ; Bellini, E. (Geneva U., Dept. Theor. Phys.) ; Benisty, D. (Cambridge U., DAMTP ; Cambridge U., KICC ; Cambridge U., Inst. of Astron.) ; Bertone, G. (Amsterdam U. ; U. Amsterdam, GRAPPA) ; Blasi, P. (GSSI, Aquila ; Gran Sasso) et al.
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. [...]
arXiv:2110.10074. - 134.
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5.
Cosmology with the Laser Interferometer Space Antenna / LISA Cosmology Working Group Collaboration
The Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological focus: to probe the expansion rate of the universe, and to understand stochastic gravitational-wave backgrounds and their implications for early universe and particle physics, from the MeV to the Planck scale. However, the range of potential cosmological applications of gravitational wave observations extends well beyond these two objectives. [...]
arXiv:2204.05434; LISA CosWG-22-03; FERMILAB-PUB-22-349-SCD.- 2023-08-28 - 176 p. - Published in : Living Rev. Relativ. 26 (2023) 5 Fulltext: jt - PDF; 2204.05434 - PDF; Fulltext from Publisher: PDF; External link: Fermilab Library Server
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6.
New horizons for fundamental physics with LISA / LISA Collaboration
The Laser Interferometer Space Antenna (LISA) has the potential to reveal wonders about the fundamental theory of nature at play in the extreme gravity regime, where the gravitational interaction is both strong and dynamical. In this white paper, the Fundamental Physics Working Group of the LISA Consortium summarizes the current topics in fundamental physics where LISA observations of GWs can be expected to provide key input. [...]
arXiv:2205.01597.- 2022-06-30 - 116 p. - Published in : Living Rev. Relativ. 25 (2022) 4 Fulltext: 2205.01597 - PDF; document - PDF;
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7.
Prospects for Fundamental Physics with LISA / LISA Collaboration
In this paper, which is of programmatic rather than quantitative nature, we aim to further delineate and sharpen the future potential of the LISA mission in the area of fundamental physics. Given the very broad range of topics that might be relevant to LISA, we present here a sample of what we view as particularly promising directions, based in part on the current research interests of the LISA scientific community in the area of fundamental physics. [...]
arXiv:2001.09793.- 2020-08-31 - 22 p. Fulltext: PDF;
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8.
Weakening Gravity on Redshift-Survey Scales with Kinetic Matter Mixing / D'Amico, Guido (CERN) ; Huang, Zhiqi (Zhongshan U.) ; Mancarella, Michele (IPhT, Saclay ; Orsay) ; Vernizzi, Filippo (IPhT, Saclay ; Orsay)
We explore general scalar-tensor models in the presence of a kinetic mixing between matter and the scalar field, which we call Kinetic Matter Mixing. In the frame where gravity is de-mixed from the scalar this is due to disformal couplings of matter species to the gravitational sector, with disformal coefficients that depend on the gradient of the scalar field. [...]
arXiv:1609.01272; CERN-TH-2016-192.- 2017 - 39 p. - Published in : JCAP 02 (2017) 014 Fulltext: PDF; External link: Preprint
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9.
$\delta N$ formalism from superpotential and holography / Garriga, Jaume (Barcelona U., Dept. Fund. Phys. ; ICC, Barcelona U. ; Tufts U., Inst. of Cosmology ; Tufts U.) ; Urakawa, Yuko (Nagoya U. ; Princeton, Inst. Advanced Study) ; Vernizzi, Filippo (CERN ; IPhT, Saclay)
We consider the superpotential formalism to describe the evolution of scalar fields during inflation, generalizing it to include the case with non-canonical kinetic terms. We provide a characterization of the attractor behaviour of the background evolution in terms of first and second slow-roll parameters (which need not be small). [...]
arXiv:1509.07339; CERN-PH-TH-2015-231; CERN-PH-TH-2015-231.- Geneva : CERN, 2016-02-16 - 38 p. - Published in : JCAP 02 (2016) 036 Article from SCOAP3: PDF; Fulltext: arXiv:1509.07339 - PDF; 10.1088_1475-7516_2016_02_036 - PDF; IOP Open Access article: PDF; External link: Preprint
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10.
Effective Theory of Dark Energy at Redshift Survey Scales / Gleyzes, Jérôme (IPhT, Saclay ; U. Paris-Sud 11, Dept. Phys., Orsay) ; Langlois, David (APC, Paris) ; Mancarella, Michele (IPhT, Saclay ; U. Paris-Sud 11, Dept. Phys., Orsay ; CERN) ; Vernizzi, Filippo (IPhT, Saclay ; CERN)
We explore the phenomenological consequences of general late-time modifications of gravity in the quasi-static approximation, in the case where cold dark matter is non-minimally coupled to the gravitational sector. Assuming spectroscopic and photometric surveys with configuration parameters similar to those of the Euclid mission, we derive constraints on our effective description from three observables: the galaxy power spectrum in redshift space, tomographic weak-lensing shear power spectrum and the correlation spectrum between the integrated Sachs-Wolfe effect and the galaxy distribution. [...]
arXiv:1509.02191; CERN-PH-TH-2015-223.- Geneva : CERN, 2016 - 38 p. - Published in : JCAP 02 (2016) 056 Fulltext: PDF; IOP Open Access article: PDF; External link: Preprint
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