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Nuclear Theory·nucl-th

Monday·March 25, 2019

7 papers—3 primary·4 cross-listed

All7Primary3Cross-lists4
  1. 04

    [Submitted on 21 Mar 2019] (cross-list from hep-ph)

    New Observables in Inclusive Production of Quarkonia

    Jean-Philippe Lansberg🇫🇷

    After an introduction motivating the study of quarkonium production, we review the recent developments in the phenomenology of quarkonium production in inclusive scatterings of hadrons and leptons. We naturally address data and predictions relevant for the LHC, the Tevatron, RHIC, HERA, LEP, B factories and EIC. An up-to-date discussion of the contributions from feed downs within the charmonium and bottomonium families as well as from b hadrons to charmonia is also provided. This contextualises an exhaustive overview of new observables such as the associated production along with a Standard Model boson (photon, W and Z), with another quarkonium, with another heavy quark as well as with light hadrons or jets. We address the relevance of these reactions in order to improve our understanding of the mechanisms underlying quarkonium production as well as the physics of multi-parton interactions, in particular the double parton scatterings. An outlook towards future studies and facilities concludes this review.

    Comments:
    LaTeX, 151 pages; 71 figures, 13 tables. Version accepted for publication in Physics Reports
    Subjects:
    High Energy Physics — Phenomenology (hep-ph); High Energy Physics — Experiment (hep-ex); Nuclear Experiment (nucl-ex); Nuclear Theory (nucl-th)
    arXiv:
    1903.09185 [pdf]
    Phys.Rept.(2020)·238 citations
  2. 05

    [Submitted on 21 Mar 2019] (cross-list from astro-ph.HE)

    Extreme Gravity and Fundamental Physics

    B.S. Sathyaprakash (Penn State and Cardiff University)🇺🇸 · Alessandra Buonanno (Max Planck Institute for Gravitational Physics, Potsdam and University of Maryland)🇩🇪 · Luis Lehner (Perimeter Institute)🇨🇦 · Chris Van Den Broeck (NIKHEF)🇳🇱 · P. Ajith (International Centre for Theoretical Sciences)🇮🇳 · Archisman Ghosh (NIKHEF)🇳🇱 · Katerina Chatziioannou (Flatiron Institute)🇺🇸 · Paolo Pani (Sapienza University of Rome)🇮🇹 · Michael Puerrer (Max Planck Institute for Gravitational Physics, Potsdam)🇩🇪 · Sanjay Reddy (Institute for Nuclear Theory, University of Washington, Seattle) · Thomas Sotiriou (The University of Nottingham)🇬🇧 · Salvatore Vitale (MIT)🇺🇸 and 17 other authors

    Future gravitational-wave observations will enable unprecedented and unique science in extreme gravity and fundamental physics answering questions about the nature of dynamical spacetimes, the nature of dark matter and the nature of compact objects.

    Comments:
    14 pages, 2 figures, White Paper submitted to the Astro-2020 (2020 Astronomy and Astrophysics Decadal Survey) by GWIC-3G Science Case Team (GWIC: Gravitational-Wave International Committee); replaced Figure 1 with a revised version that incorporates Gravity IR Flare data point
    Subjects:
    High Energy Astrophysical Phenomena (astro-ph.HE); General Relativity and Quantum Cosmology (gr-qc); High Energy Physics — Theory (hep-th); Nuclear Theory (nucl-th)
    arXiv:
    1903.09221 [pdf]
    96 citations
  3. 06

    [Submitted on 21 Mar 2019] (cross-list from astro-ph.HE)

    The Yet-Unobserved Multi-Messenger Gravitational-Wave Universe

    Vassiliki Kalogera (Northwestern U.)🇺🇸 · Marrie-Anne Bizouard (CNRS, OCA)🇫🇷 · Adam Burrows (Princeton U.)🇺🇸 · Thomas Janka (MPA)🇩🇪 · Kei Kotake (Fukuoka U.)🇯🇵 · Bronson Messer (ORNL \& U. Tennessee)🇺🇸 · Tony Mezzacappa (ORNL & U. Tennessee)🇺🇸 · Bernhard Mueller (Monash U.)🇦🇺 · Ewald Mueller (MPA)🇩🇪 · Maria Alessandra Papa (AEI)🇩🇪 · Sanjay Reddy (U. Washington)🇺🇸 · Stephan Rosswog (Stockholms U.)🇸🇪

    Observations with next-generation ground-based detectors further enhanced with multi-messenger (electromagnetic and neutrino) detections will allow us to probe new extreme astrophysics. Target sources included: core-collapse supernovae, continuous emission from isolated or accreting neutron stars, and bursts from magnetars and other pulsars.

    Comments:
    13 pages, 1 figure, White Paper Submitted to Astro2020 (2020 Astronomy and Astrophysics Decadal Survey) by GWIC 3G Science Case Team (GWIC: Gravitational Wave International Committee)
    Subjects:
    High Energy Astrophysical Phenomena (astro-ph.HE); General Relativity and Quantum Cosmology (gr-qc); Nuclear Theory (nucl-th)
    arXiv:
    1903.09224 [pdf]
    15 citations
  4. 07

    [Submitted on 22 Mar 2019] (cross-list from astro-ph.HE)

    Multimessenger Universe with Gravitational Waves from Binaries

    B.S. Sathyaprakash (Penn State and Cardiff University)🇺🇸 · Matthew Bailes (Swinburne U.)🇦🇺 · Mansi M. Kasliwal (Caltech)🇺🇸 · Samaya Nissanke (U. of Amsterdam)🇳🇱 · Shreya Anand (Caltech)🇺🇸 · Igor Andreoni (Caltech)🇺🇸 · Monica Colpi (U. of Milano - Bicocca)🇮🇹 · Michael Coughlin (Caltech)🇺🇸 · Evan Hall (MIT)🇺🇸 · Vicky Kalogera (Northwestern U.)🇺🇸 · Dan Kasen (UC Berkeley)🇺🇸 · Alberto Sesana (U. Birmingham)🇬🇧

    Future GW detector networks and EM observatories will provide a unique opportunity to observe the most luminous events in the Universe involving matter in extreme environs. They will address some of the key questions in physics and astronomy: formation and evolution of compact binaries, sites of formation of heavy elements and the physics of jets.

    Comments:
    11 pages, two tables, White Paper submitted to the Astro-2020 (2020 Astronomy and Astrophysics Decadal Survey) by GWIC-3G Science Case Team (GWIC: Gravitational-Wave International Committee)
    Subjects:
    High Energy Astrophysical Phenomena (astro-ph.HE); Nuclear Theory (nucl-th)
    arXiv:
    1903.09277 [pdf]
    19 citations

Affiliations

first authorsco-authorsvia INSPIRE