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Publikováno v:
Chinese Physics
In this paper, we calculate the $t\bar{t}$ pQCD production cross-section at NNLO and determine the top-quark pole mass from recent measurements at the LHC at $\sqrt{S}=13$ TeV center-of-mass energy to high precision by applying the Principle of Maxim
Publikováno v:
Letters in High Energy Physics, Vol 2021, Iss 1 (2021)
The \(K_S-K_L\) (SL) asymmetry occurs in the two-body charmed baryon decay with neutral kaon contained in their final states.In this work, based on the topological diagram approach and separated contributions calculated in naive factorization and the
Autor:
Yoritaka Iwata, Shahariar Sarkar
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 8 (2021)
In the present work, the λ mechanism (left-right weak boson exchange) and the light neutrino-exchange mechanism of neutrinoless double beta decay is studied. In particular, much attention is paid to the calculation of nuclear matrix elements for one
Publikováno v:
Chinese Physics
We apply an equal-velocity quark combination model to study the production of light-flavor hadrons and single-charmed hadrons at midrapidity in $pp$ collisions at $\sqrt{s}=5.02$ TeV. We find experimental data for $p_{T}$ spectra of $\Omega$ and $\ph
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 494:2076-2089
Standard analysis pipelines for measurements of Baryon Acoustic Oscillations (BAO) in galaxy surveys make use of a fiducial cosmological model to guide the data compression required to transform from observed redshifts and angles to the measured angu
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 493 (4), pp.5257-5272. ⟨10.1093/mnras/staa405⟩
Monthly Notices of the Royal Astronomical Society, 2020, 493 (4), pp.5257-5272. ⟨10.1093/mnras/staa405⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 493 (4), pp.5257-5272. ⟨10.1093/mnras/staa405⟩
Monthly Notices of the Royal Astronomical Society, 2020, 493 (4), pp.5257-5272. ⟨10.1093/mnras/staa405⟩
We use mock galaxy data from the VIMOS Public Extragalactic Redshift Survey (VIPERS) to test the performance of the Multi-Tracer Optimal Estimator (MTOE) of Abramo et al. as a tool to measure the monopoles of the power spectra of multiple tracers of
Autor:
Jens Chluba, Luke Hart
Publikováno v:
Hart, L & Chluba, J 2020, ' Updated fundamental constant constraints from Planck 2018 data and possible relations to the Hubble tension ', Monthly Notices of the Royal Astronomical Society, vol. 493, no. 3, pp. 3255-3263 . https://doi.org/10.1093/mnras/staa412
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society
We present updated constraints on the variation of the fine structure constant, $\alpha_{\rm EM}$, and effective electron rest mass, $m_{\rm e}$, during the cosmological recombination era. These two fundamental constants directly affect the ionizatio
Autor:
G. S. Hajyan
Publikováno v:
Astrophysics. 63:125-132
The MIT quark bag model is used to determine the thermodynamic characteristics of hot strange quark matter that is opaque to neutrinos. Three different variants of the lepton content of hot quark matter are considered. The numerical calculations are
Autor:
Antony Lewis, X. Dupac, James R. Fergusson, François R. Bouchet, Diego Molinari, E. Martínez-González, Jean-François Cardoso, L. Salvati, Jörg P. Rachen, Krzysztof M. Gorski, K. Ganga, A. Marcos-Caballero, C. Combet, Hannu Kurki-Suonio, E. Di Valentino, Jose M. Diego, L. Montier, Jan Hamann, J. F. Macías-Pérez, E. Franceschi, Charles R. Lawrence, M. Douspis, Erminia Calabrese, E. P. S. Shellard, Frederico Arroja, M. Le Jeune, P. Vielva, Andrea Zacchei, Graca Rocha, Martina Gerbino, Zhiqi Huang, Davide Maino, Adam Moss, Ricardo Genova-Santos, D. Tavagnacco, M. López-Caniego, A. A. Fraisse, M. Tenti, F. Piacentini, J.-P. Bernard, P. de Bernardis, Tiziana Trombetti, L. Toffolatti, Soumen Basak, F. Elsner, J.-L. Puget, Benjamin D. Wandelt, Julian Borrill, R. B. Barreiro, Gabriel Jung, Michele Liguori, S. Galeotta, Will Handley, F. Cuttaia, G. Polenta, R. C. Butler, K. Kiiveri, Anthony Lasenby, Alessandro Melchiorri, Reijo Keskitalo, A. J. Banday, M.-A. Miville-Deschênes, A. Renzi, P. Bielewicz, F. Oppizzi, Yashar Akrami, Anthony Challinor, B. Casaponsa, E. Keihänen, Gianmarco Maggio, B. P. Crill, Nicola Bartolo, B. Van Tent, Fabrizio Villa, Francesca Perrotta, F. K. Hansen, J. B. Kim, G. Sirri, Andrei V. Frolov, Michele Maris, J. A. Tauber, M. Savelainen, D. Herranz, A.-S. Suur-Uski, Yabebal Fantaye, Sabino Matarrese, M. Migliaccio, M. Tomasi, M. Bucher, Nicola Vittorio, J. Valiviita, V. Lindholm, W. C. Jones, Douglas Scott, R. Fernandez-Cobos, D. Paoletti, Marco Bersanelli, Torsten A. Enßlin, A. Moneti, M. Frailis, Carlo Baccigalupi, V. Pettorino, François Levrier, E. Hivon, J. Aumont, B. Racine, A. Mennella, G. Patanchon, Alessandro Gruppuso, Ingunn Kathrine Wehus, M. Reinecke, J.-M. Delouis, P. D. Meerburg, Massimiliano Lattanzi, Jose Alberto Rubino-Martin, N. Mandolesi, Chiara Sirignano, Kendrick M. Smith, Andrew H. Jaffe, Peter Meinhold, J.-M. Lamarre, A. de Rosa, G. de Zotti, B. Partridge, J. González-Nuevo, A. Ducout, Locke D. Spencer, M. Ashdown, H. K. Eriksen, Martin Kunz, Mathieu Remazeilles, Jon E. Gudmundsson, L. P. L. Colombo, Jason D. McEwen, Mario Ballardini, Peter G. Martin, George Efstathiou, Serge Gratton, Carlo Burigana, Nicoletta Krachmalnicoff, Yin-Zhe Ma, Jacques Delabrouille, Fabio Finelli, L. Pagano, N. Mauri, S. Dusini, Andrea Zonca, R. A. Sunyaev, P. B. Lilje, Luca Stanco, H. C. Chiang, K. Benabed, J. R. Bond, B. Ruiz-Granados, O. Doré, Paolo Natoli, Maresuke Shiraishi, Moritz Münchmeyer, S. Galli, Gianluca Morgante
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 641, pp.A9. ⟨10.1051/0004-6361/201935891⟩
Astronomy & Astrophysics, 641, pp. 1-47
Astronomy & Astrophysics, 641, 1-47
Scopus
Astronomy & Astrophysics. Vol 641, sep. 2020. A9
UCrea Repositorio Abierto de la Universidad de Cantabria
Universidad de Cantabria (UC)
Astronomy & Astrophysics (0004-6361) (Edp Sciences S A), 2020-09, Vol. 641, N. A9, P. 47p.
Astronomy and astrophysics, 641:A9. EDP Sciences
RUO. Repositorio Institucional de la Universidad de Oviedo
instname
Digital.CSIC. Repositorio Institucional del CSIC
Astronomy and Astrophysics-A&A, 2020, 641, pp.A9. ⟨10.1051/0004-6361/201935891⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 641, pp.A9. ⟨10.1051/0004-6361/201935891⟩
Astronomy & Astrophysics, 641, pp. 1-47
Astronomy & Astrophysics, 641, 1-47
Scopus
Astronomy & Astrophysics. Vol 641, sep. 2020. A9
UCrea Repositorio Abierto de la Universidad de Cantabria
Universidad de Cantabria (UC)
Astronomy & Astrophysics (0004-6361) (Edp Sciences S A), 2020-09, Vol. 641, N. A9, P. 47p.
Astronomy and astrophysics, 641:A9. EDP Sciences
RUO. Repositorio Institucional de la Universidad de Oviedo
instname
Digital.CSIC. Repositorio Institucional del CSIC
Astronomy and Astrophysics-A&A, 2020, 641, pp.A9. ⟨10.1051/0004-6361/201935891⟩
Planck Collaboration: et al.
arXiv:1905.05697v1
We analyse the Planck full-mission cosmic microwave background (CMB) temperature and E-mode polarization maps to obtain constraints on primordial non-Gaussianity (NG). We compare estimates obt
arXiv:1905.05697v1
We analyse the Planck full-mission cosmic microwave background (CMB) temperature and E-mode polarization maps to obtain constraints on primordial non-Gaussianity (NG). We compare estimates obt
Publikováno v:
Astroparticle Physics. 114:80-91
Assuming for Weakly Interacting Massive Particles (WIMPs) a Maxwellian velocity distribution in the Galaxy we provide an assessment of the sensitivity of existing Dark Matter (DM) direct detection (DD) experiments to operators up to dimension 7 of th