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Gravitational waves from cosmic strings in LISA: reconstruction pipeline and physics interpretation
/ Blanco-Pillado, Jose J. (IKERBASQUE, Bilbao ; Basque U., Bilbao ; U. Basque Country, Leioa) ; Cui, Yanou (UC, Riverside) ; Kuroyanagi, Sachiko (Madrid, IFT ; Nagoya U.) ; Lewicki, Marek (Warsaw U.) ; Nardini, Germano (Stavanger U.) ; Pieroni, Mauro (CERN) ; Rybak, Ivan Yu. (Zaragoza U. ; Porto U., Astron. Dept.) ; Sousa, Lara (Porto U., Astron. Dept.) ; Wachter, Jeremy M. (Wentworth Inst. Tech.)
We initiate the LISA template databank for stochastic gravitational wave backgrounds sourced by cosmic strings. [...]
arXiv:2405.03740 ; LISA-COSWG-24-02 ; CERN-TH-2024-085.
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61 p.
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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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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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Euclid preparation. Sensitivity to non-standard particle dark matter model
/ Euclid Collaboration
The Euclid mission of the European Space Agency will provide weak gravitational lensing and galaxy clustering surveys that can be used to constrain the standard cosmological model and its extensions, with an opportunity to test the properties of dark matter beyond the minimal cold dark matter paradigm. [...]
arXiv:2406.18274 ; TTK-24-26.
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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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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.
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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.
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Local Probing Of Ferroic And Multiferroic Compounds
/ Lopes, A M L (IFIMUP-IN, Fac. Ciências, Univ. Porto, P-4150 Porto, Portugal) ; Schell, Juliana (Institute for Materials Science and Center for Nanointegration, Duisburg-Essen (CENIDE), University of Duisburg-Essen) ; Amaral, V S (Dep. Physics and CICECO, Univ. Aveiro, P-3810-193 Aveiro, Portugal) ; Amorim, C O (Dep. Physics and CICECO, Univ. Aveiro, P-3810-193 Aveiro, Portugal) ; Araújo, J P (IFIMUP, Fac. Ciências, Univ. Porto, P-4150 Porto, Portugal) ; Baghizadeh, A (Dep. Mat & Cer. Eng. and CICECO, Univ. Aveiro, P-3810-193 Aveiro, Portugal) ; Baptista, M (IFIMUP, Fac. Ciências, Univ. Porto, P-4150 Porto, Portugal) ; Becker, Hans-Werner (Ruhr-Universität Bochum, RUBION, Universitätsstr. 150, D-44801 Bochum) ; Correia, J G (C2TN, Centro de Ciências e Tecnologias Nucleares, Instituto Superior Técnico, Universidade de Lisboa, Portugal) ; Escobar Castillo, M (Institute for Materials Science and Center for Nanointegration, Duisburg-Essen (CENIDE), University of Duisburg-Essen, 45141 Essen, Germany) et al.
CERN-INTC-2017-074 ; INTC-CLL-034.
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