CERN Accelerating science

CERN Document Server 14 のレコードが見つかりました。  1 - 10次  レコードへジャンプ: 検索にかかった時間: 0.64 秒 
1.
Extended Analysis of Neutrino-Dark Matter Interactions with Small-Scale CMB Experiments / Brax, Philippe (IPhT, Saclay ; CERN) ; van de Bruck, Carsten (Sheffield U.) ; Di Valentino, Eleonora (Sheffield U.) ; Giarè, William (Sheffield U.) ; Trojanowski, Sebastian (Warsaw, Copernicus Astron. Ctr. ; NCBJ, Warsaw)
We explore an extension of the standard $\Lambda$CDM model by including an interaction between neutrinos and dark matter, and making use of the ground based telescope data of the Cosmic Microwave Background (CMB) from the Atacama Cosmology Telescope (ACT). An indication for a non-zero coupling between dark matter and neutrinos (both assuming a temperature independent and $T^2$ dependent cross-section) is obtained at the 1$\sigma$ level coming from the ACT CMB data alone and when combined with the Planck CMB and Baryon Acoustic Oscillations (BAO) measurements. [...]
arXiv:2305.01383.- 2023-08-30 - 14 p. - Published in : Phys. Dark Univ. 42 (2023) 101321 Fulltext: Publication - PDF; 2305.01383 - PDF;
2.
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.
- 17 p.
Fulltext
3.
New insights on $\nu$-DM Interactions / Brax, Philippe (IPhT, Saclay ; CERN) ; van de Bruck, Carsten (CERN) ; Di Valentino, Eleonora (CERN) ; Giarè, William (CERN) ; Trojanowski, Sebastian (Warsaw, Copernicus Astron. Ctr. ; NCBJ, Warsaw)
We revisit the possibility of using cosmological observations to constrain models that involve interactions between neutrinos and dark matter. We show that small-scale measurements of the cosmic microwave background with a few per cent accuracy are critical to uncover unique signatures from models with tiny couplings that would require a much higher sensitivity at lower multipoles, such as those probed by the Planck satellite. [...]
arXiv:2303.16895.- 2023-10-04 - 5 p. - Published in : Mon. Not. R. Astron. Soc. 527 (2023) L122-L126 Fulltext: document - PDF; Publication - PDF; 2303.16895 - PDF;
4.
CORFU2023: 23rd Hellenic School and Workshops on Elementary Particle Physics and Gravity (CORFU 2023) - CORFU2023   23 Apr - 1 Oct 2023  - Corfu, Greece  / Agathos, Michalis (ed.) (KICC/DAMTP - U Cambridge); Anagnostopoulos, Konstantinos (ed.) (NTU Athens); Aschieri, Paolo (ed.) (U. del Piemonte Orientale); Basilakos, Spyros (ed.) (National Observatory of Athens); Capozziello, Salvatore (ed.) (U Napoli); Cardoso, Vitor (ed.) (NBI - U Copenhagen, IST Lisbon); Chatzistavrakidis, Athanassios (ed.) (Bošković Institute); Di Valentino, Eleonora (ed.) (U Sheffield); Gnecchi, Alessandra (ed.) (INFN, Padova); Kalinowski, Jan (ed.) (Warsaw U.) et al.
2023 - Published in : PoS: CORFU2024 (2024)
5.
Report of the Topical Group on Cosmic Probes of Fundamental Physics for for Snowmass 2021 / Adhikari, Rana X. (Caltech) ; Anchordoqui, Luis A. (Lehman Coll. ; City Coll., N.Y. ; Amer. Museum Natural Hist.) ; Fang, Ke (Wisconsin U., Madison) ; Sathyaprakash, B.S. (Penn State U., University Park, IGC ; Penn State U., Astron. Astrophys. ; Cardiff U.) ; Tollefson, Kirsten (Michigan State U.) ; Lewis, Tiffany R. (NASA, Goddard) ; Engel, Kristi (Maryland U. ; Los Alamos) ; Aboubrahim, Amin (U. Munster) ; Akarsu, Ozgur (Istanbul, Tech. U.) ; Akrami, Yashar (Case Western Reserve U.) et al.
Cosmic Probes of Fundamental Physics take two primary forms: Very high energy particles (cosmic rays, neutrinos, and gamma rays) and gravitational waves. [...]
arXiv:2209.11726.
- 118.
Fulltext
6.
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.
- 24 p.
Fulltext - Fulltext
7.
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.
- 2019. - 11 p.
Fulltext
8.
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;
9.
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;
10.
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;

CERN Document Server : 14 のレコードが見つかりました。   1 - 10次  レコードへジャンプ:
Interested in being notified about new results for this query?
Set up a personal email alert or subscribe to the RSS feed.
捜していたものを見つけなかったならば、他のサーバーもお試しください:
Di Valentino, E. 中の Amazon
Di Valentino, E. 中の CERN EDMS
Di Valentino, E. 中の CERN Intranet
Di Valentino, E. 中の CiteSeer
Di Valentino, E. 中の Google Books
Di Valentino, E. 中の Google Scholar
Di Valentino, E. 中の Google Web
Di Valentino, E. 中の IEC
Di Valentino, E. 中の IHS
Di Valentino, E. 中の INSPIRE
Di Valentino, E. 中の ISO
Di Valentino, E. 中の KISS Books/Journals
Di Valentino, E. 中の KISS Preprints
Di Valentino, E. 中の NEBIS
Di Valentino, E. 中の SLAC Library Catalog
Di Valentino, E. 中の Scirus