检索结果-内蒙古大学图书馆

All-sky search for continuous gravitational waves from isolated neutron stars in the early O3 LIGO data

physical Review d 2021年第8期104卷 082004-082004页

作者： R. Abbott T. d. Abbott S. Abraham F. Acernese K. Ackley A. Adams C. Adams R. X. Adhikari V. B. Adya C. Affeldt d. Agarwal M. Agathos K. Agatsuma N. Aggarwal O. d. Aguiar L. Aiello A. Ain P. Ajith T. Akutsu K. M. Aleman G. Allen A. Allocca P. A. Altin A. Amato S. Anand A. Ananyeva S. B. Anderson W. G. Anderson M. Ando S. V. Angelova S. Ansoldi J. M. Antelis S. Antier S. Appert Koya Arai Koji Arai Y. Arai S. Araki A. Araya M. C. Araya J. S. Areeda M. Arène N. Aritomi N. Arnaud S. M. Aronson H. Asada Y. Asali G. Ashton Y. Aso S. M. Aston P. Astone F. Aubin P. Aufmuth K. AultONeal C. Austin S. Babak F. Badaracco M. K. M. Bader S. Bae Y. Bae A. M. Baer S. Bagnasco Y. Bai L. Baiotti J. Baird R. Bajpai M. Ball G. Ballardin S. W. Ballmer M. Bals A. Balsamo G. Baltus S. Banagiri d. Bankar R. S. Bankar J. C. Barayoga C. Barbieri B. C. Barish d. Barker P. Barneo F. Barone B. Barr L. Barsotti M. Barsuglia d. Barta J. Bartlett M. A. Barton I. Bartos R. Bassiri A. Basti M. Bawaj J. C. Bayley A. C. Baylor M. Bazzan B. Bécsy V. M. Bedakihale M. Bejger I. Belahcene V. Benedetto d. Beniwal M. G. Benjamin T. F. Bennett J. d. Bentley M. BenYaala F. Bergamin B. K. Berger S. Bernuzzi d. Bersanetti A. Bertolini J. Betzwieser R. Bhandare A. V. Bhandari d. Bhattacharjee S. Bhaumik J. Bidler I. A. Bilenko G. Billingsley R. Birney O. Birnholtz S. Biscans M. Bischi S. Biscoveanu A. Bisht B. Biswas M. Bitossi M.-A. Bizouard J. K. Blackburn J. Blackman C. d. Blair d. G. Blair R. M. Blair F. Bobba N. Bode M. Boer G. Bogaert M. Boldrini F. Bondu E. Bonilla R. Bonnand P. Booker B. A. Boom R. Bork V. Boschi N. Bose S. Bose V. Bossilkov V. Boudart Y. Bouffanais A. Bozzi C. Bradaschia P. R. Brady A. Bramley A. Branch M. Branchesi J. E. Brau M. Breschi T. Briant J. H. Briggs A. Brillet M. Brinkmann P. Brockill A. F. Brooks J. Brooks d. d. Brown S. Brunett G. Bruno R. Bruntz J. Bryant A. Buikema T. Bulik H. J. Bulten A. Buonanno R. Buscicchio d. Buskulic R. L. Byer L. Cadonati M. Caesar G. Cagnoli C. Cahillane H. W. Cain, III J. Calderón Bustillo J. LIGO Laboratory California Institute of Technology Pasadena California 91125 USA Louisiana State University Baton Rouge Louisiana 70803 USA Inter-University Centre for Astronomy and Astrophysics Pune 411007 India Dipartimento di Farmacia Università di Salerno I-84084 Fisciano Salerno Italy INFN Sezione di Napoli Complesso Universitario di Monte S.Angelo I-80126 Napoli Italy OzGrav School of Physics and Astronomy Monash University Clayton 3800 Victoria Australia Christopher Newport University Newport News Virginia 23606 USA LIGO Livingston Observatory Livingston Louisiana 70754 USA OzGrav Australian National University Canberra Australian Capital Territory 0200 Australia Max Planck Institute for Gravitational Physics (Albert Einstein Institute) D-30167 Hannover Germany Leibniz Universität Hannover D-30167 Hannover Germany University of Cambridge Cambridge CB2 1TN United Kingdom Theoretisch-Physikalisches Institut Friedrich-Schiller-Universität Jena D-07743 Jena Germany University of Birmingham Birmingham B15 2TT United Kingdom Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA) Northwestern University Evanston Illinois 60208 USA Instituto Nacional de Pesquisas Espaciais 12227-010 São José dos Campos São Paulo Brazil Gravity Exploration Institute Cardiff University Cardiff CF24 3AA United Kingdom Gran Sasso Science Institute (GSSI) I-67100 L’Aquila Italy INFN Laboratori Nazionali del Gran Sasso I-67100 Assergi Italy INFN Sezione di Pisa I-56127 Pisa Italy Università di Pisa I-56127 Pisa Italy International Centre for Theoretical Sciences Tata Institute of Fundamental Research Bengaluru 560089 India Gravitational Wave Science Project National Astronomical Observatory of Japan (NAOJ) Mitaka City Tokyo 181-8588 Japan Advanced Technology Center National Astronomical Observatory of Japan (NAOJ) Mitaka City Tokyo 181-8588 Japan California State University Fullerton Fullerton California 92831 USA NCSA University of Illi

We report on an all-sky search for continuous gravitational waves in the frequency band 20–2000 Hz and with a frequency time derivative in the range of [−1.0,+0.1]×10−8 Hz/s. Such a signal could be produced by a nearby, spinning and slightly nonaxisymmetric isolated neutron star in our Galaxy. This search uses the LIGO data from the first six months of Advanced LIGO’s and Advanced Virgo’s third observational run, O3. No periodic gravitational wave signals are observed, and 95% confidence-level (C.L.) frequentist upper limits are placed on their strengths. The lowest upper limits on worst-case (linearly polarized) strain amplitude h0 are ∼1.7×10−25 near 200 Hz. For a circularly polarized source (most favorable orientation), the lowest upper limits are ∼6.3×10−26. These strict frequentist upper limits refer to all sky locations and the entire range of frequency derivative values. For a population-averaged ensemble of sky locations and stellar orientations, the lowest 95% C.L. upper limits on the strain amplitude are ∼1.4×10−25. These upper limits improve upon our previously published all-sky results, with the greatest improvement (factor of ∼2) seen at higher frequencies, in part because quantum squeezing has dramatically improved the detector noise level relative to the second observational run, O2. These limits are the most constraining to date over most of the parameter space searched.

关键词： Astrophysical studies of gravity Gravitational wave detection Gravitational wave sources Gravitational waves

来源：评论

学校读者我要写书评

暂无评论

Upper limits on the isotropic gravitational-wave background from Advanced LIGO and Advanced Virgo’s third observing run

引用

physical Review d 2021年第2期104卷 022004-022004页

作者： R. Abbott T. d. Abbott S. Abraham F. Acernese K. Ackley A. Adams C. Adams R. X. Adhikari V. B. Adya C. Affeldt d. Agarwal M. Agathos K. Agatsuma N. Aggarwal O. d. Aguiar L. Aiello A. Ain T. Akutsu K. M. Aleman G. Allen A. Allocca P. A. Altin A. Amato S. Anand A. Ananyeva S. B. Anderson W. G. Anderson M. Ando S. V. Angelova S. Ansoldi J. M. Antelis S. Antier S. Appert Koya Arai Koji Arai Y. Arai S. Araki A. Araya M. C. Araya J. S. Areeda M. Arène N. Aritomi N. Arnaud S. M. Aronson H. Asada Y. Asali G. Ashton Y. Aso S. M. Aston P. Astone F. Aubin P. Aufmuth K. AultONeal C. Austin S. Babak F. Badaracco M. K. M. Bader S. Bae Y. Bae A. M. Baer S. Bagnasco Y. Bai L. Baiotti J. Baird R. Bajpai M. Ball G. Ballardin S. W. Ballmer M. Bals A. Balsamo G. Baltus S. Banagiri d. Bankar R. S. Bankar J. C. Barayoga C. Barbieri B. C. Barish d. Barker P. Barneo S. Barnum F. Barone B. Barr L. Barsotti M. Barsuglia d. Barta J. Bartlett M. A. Barton I. Bartos R. Bassiri A. Basti M. Bawaj J. C. Bayley A. C. Baylor M. Bazzan B. Bécsy V. M. Bedakihale M. Bejger I. Belahcene V. Benedetto d. Beniwal M. G. Benjamin T. F. Bennett J. d. Bentley M. BenYaala F. Bergamin B. K. Berger S. Bernuzzi d. Bersanetti A. Bertolini J. Betzwieser R. Bhandare A. V. Bhandari d. Bhattacharjee S. Bhaumik J. Bidler I. A. Bilenko G. Billingsley R. Birney O. Birnholtz S. Biscans M. Bischi S. Biscoveanu A. Bisht B. Biswas M. Bitossi M.-A. Bizouard J. K. Blackburn J. Blackman C. d. Blair d. G. Blair R. M. Blair F. Bobba N. Bode M. Boer G. Bogaert M. Boldrini F. Bondu E. Bonilla R. Bonnand P. Booker B. A. Boom R. Bork V. Boschi N. Bose S. Bose V. Bossilkov V. Boudart Y. Bouffanais A. Bozzi C. Bradaschia P. R. Brady A. Bramley A. Branch M. Branchesi J. E. Brau M. Breschi T. Briant J. H. Briggs A. Brillet M. Brinkmann P. Brockill A. F. Brooks J. Brooks d. d. Brown S. Brunett G. Bruno R. Bruntz J. Bryant A. Buikema T. Bulik H. J. Bulten A. Buonanno R. Buscicchio d. Buskulic R. L. Byer L. Cadonati M. Caesar G. Cagnoli C. Cahillane H. W. Cain, III J. Calderón Bustillo J. LIGO Laboratory California Institute of Technology Pasadena California 91125 USA Louisiana State University Baton Rouge Louisiana 70803 USA Inter-University Centre for Astronomy and Astrophysics Pune 411007 India Dipartimento di Farmacia Università di Salerno I-84084 Fisciano Salerno Italy INFN Sezione di Napoli Complesso Universitario di Monte S. Angelo I-80126 Napoli Italy OzGrav School of Physics & Astronomy Monash University Clayton 3800 Victoria Australia Christopher Newport University Newport News Virginia 23606 USA LIGO Livingston Observatory Livingston Louisiana 70754 USA OzGrav Australian National University Canberra Australian Capital Territory 0200 Australia Max Planck Institute for Gravitational Physics (Albert Einstein Institute) D-30167 Hannover Germany Leibniz Universität Hannover D-30167 Hannover Germany University of Cambridge Cambridge CB2 1TN United Kingdom Theoretisch-Physikalisches Institut Friedrich-Schiller-Universität Jena D-07743 Jena Germany University of Birmingham Birmingham B15 2TT United Kingdom Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA) Northwestern University Evanston Illinois 60208 USA Instituto Nacional de Pesquisas Espaciais 12227-010 São José dos Campos São Paulo Brazil Gravity Exploration Institute Cardiff University Cardiff CF24 3AA United Kingdom Gran Sasso Science Institute (GSSI) I-67100 L’Aquila Italy INFN Laboratori Nazionali del Gran Sasso I-67100 Assergi Italy INFN Sezione di Pisa I-56127 Pisa Italy Università di Pisa I-56127 Pisa Italy Gravitational Wave Science Project National Astronomical Observatory of Japan (NAOJ) Mitaka City Tokyo 181-8588 Japan Advanced Technology Center National Astronomical Observatory of Japan (NAOJ) Mitaka City Tokyo 181-8588 Japan California State University Fullerton Fullerton California 92831 USA NCSA University of Illinois at Urbana-Champaign Urbana Illinois 61801 USA Università di Napoli “Federico II” Complesso Universitario

We report results of a search for an isotropic gravitational-wave background (GWB) using data from Advanced LIGO’s and Advanced Virgo’s third observing run (O3) combined with upper limits from the earlier O1 and O2 runs. Unlike in previous observing runs in the advanced detector era, we include Virgo in the search for the GWB. The results of the search are consistent with uncorrelated noise, and therefore we place upper limits on the strength of the GWB. We find that the dimensionless energy density ΩGW≤5.8×10−9 at the 95% credible level for a flat (frequency-independent) GWB, using a prior which is uniform in the log of the strength of the GWB, with 99% of the sensitivity coming from the band 20–76.6 Hz; ΩGW(f)≤3.4×10−9 at 25 Hz for a power-law GWB with a spectral index of 2/3 (consistent with expectations for compact binary coalescences), in the band 20–90.6 Hz; and ΩGW(f)≤3.9×10−10 at 25 Hz for a spectral index of 3, in the band 20–291.6 Hz. These upper limits improve over our previous results by a factor of 6.0 for a flat GWB, 8.8 for a spectral index of 2/3, and 13.1 for a spectral index of 3. We also search for a GWB arising from scalar and vector modes, which are predicted by alternative theories of gravity; we do not find evidence of these, and place upper limits on the strength of GWBs with these polarizations. We demonstrate that there is no evidence of correlated noise of magnetic origin by performing a Bayesian analysis that allows for the presence of both a GWB and an effective magnetic background arising from geophysical Schumann resonances. We compare our upper limits to a fiducial model for the GWB from the merger of compact binaries, updating the model to use the most recent data-driven population inference from the systems detected during O3a. Finally, we combine our results with observations of individual mergers and show that, at design sensitivity, this joint approach may yield stronger constraints on the merger rate of binary black holes at z≳2

关键词： Gravitational wave detection

来源：评论

学校读者我要写书评

暂无评论

Effect of mouth-opening levels on sound field gain in the ear canal 45

Effect of mouth-opening levels on sound field gain in the ea...

引用

45th International Congress and Exposition on Noise Control engineering: Towards a Quieter Future, INTER-NOISE 2016

作者： Xiao, Jimg-Hong Yu, Jen-Fang Lee, Kun-Che Chiu, Hsiu-Hui Graduate Institute of Medical Mechatronics Chang Gung University Taiwan Taiouan Interdisciplinary Otolaryngology Laboratory Chang Gung University Taiwan Ph.D. Program in Biomedical Engineering College of Engineering Chang Gung University Taiwan

The human ear canal can become deformed when the mouth opens and closes, changing the sound field in the external auditory canal. Thus, measuring the mandibular movement trajectory may provide a reference for identifying mouth-opening levels. The human ear canal can become deformed when the mouth opens and closes, changing the sound field in the external auditory canal. Thus, measuring the mandibular movement trajectory may provide a reference for identifying mouth-opening levels. The K7 system and a Frye Fonix 7000 sensor were used to perform several measurements of mouth-opening and -closing to obtain the mean maximal mouth opening level. The mandible was fixed at the 1/3, 2/3, and maximal mouth-opening levels. Subsequently, a 65-dB sweep tone, which is the sound pressure level of people talking at a normal level, was adopted as the sound stimulus to measure sound fields at 5, 10, 15, and 20 mm from the entrance of the external auditory canal. The stimulus frequencies of 200, 500, 1000, 2000, 4000, 6000, and 8000 Hz were noted. The differences in sound field gains at depths of 5, 10, 15, and 20 mm were analyzed for the various mouth-opening levels. The results show that except for the 1.70-dB decrease at a depth of 5 mm with an 8000-Hz stimulus frequency, the differences at the other depths and stimulus frequencies were within 1 dB. Thus, the mouth-opening levels will influence the gain in ear canal. © 2016, German Acoustical Society (dEGA). All rights reserved.

关键词： Acoustic fields

来源：评论

学校读者我要写书评

暂无评论

First Constraints on the Epoch of Reionization Using the non-Gaussianity of the Kinematic Sunyaev-Zel’dovich Effect from the South Pole Telescope and Herschel-SPIRE Observations

arXiv

引用

arXiv 2024年

作者： Raghunathan, S. Ade, P.A.R. Anderson, A.J. Ansarinejad, B. Archipley, M. Austermann, J.E. Balkenhol, L. Beall, J.A. Benabed, K. Bender, A.N. Benson, B.A. Bianchini, F. Bleem, L.E. Bock, J. Bouchet, F.R. Bryant, L. Camphuis, E. Carlstrom, J.E. Cecil, T.W. Chang, C.L. Chaubal, P. Chiang, H.C. Chichura, P.M. Chou, T.-L. Citron, R. Coerver, A. Crawford, T.M. Crites, A.T. Cukierman, A. daley, C. dibert, K.R. dobbs, M.A. doussot, A. dutcher, d. Everett, W. Feng, C. Ferguson, K.R. Fichman, K. Foster, A. Galli, S. Gallicchio, J. Gambrel, A.E. Gardner, R.W. Ge, F. George, E.M. Goeckner-Wald, N. Gualtieri, R. Guidi, F. Guns, S. Gupta, N. de Haan, T. Halverson, N.W. Hivon, E. Holder, G.P. Holzapfel, W.L. Hood, J.C. Hrubes, J.d. Hryciuk, A. Huang, N. Hubmayr, J. Irwin, K.d. Kéruzoré, F. Khalife, A.R. Knox, L. Korman, M. Kornoelje, K. Kuo, C.-L. Lee, A.T. Levy, K. Li, d. Lowitz, A.E. Lu, C. Maniyar, A. Martsen, E.S. McMahon, J.J. Menanteau, F. Millea, M. Montgomery, J. Moran, C. Corbett Nakato, Y. Natoli, T. Nibarger, J.P. Noble, G.I. Novosad, V. Omori, Y. Padin, S. Pan, Z. Paschos, P. Patil, S. ph.d.e, K.A. Prabhu, K. Pryke, C. Quan, W. Rahimi, M. Rahlin, A. Reichardt, C.L. Rouble, M. Ruhl, J.E. Saliwanchik, B.R. Schaffer, K.K. Schiappucci, E. Sievers, C. Smecher, G. Sobrin, J.A. Stark, A.A. Stephen, J. Suzuki, A. Tandoi, C. Thompson, K.L. Thorne, B. Trendafilova, C. Tucker, C. Umilta, C. Veach, T. Vieira, J.d. Viero, M.P. Wan, Y. Wang, G. Whitehorn, N. Wu, W.L.K. Yefremenko, V. Young, M.R. Zebrowski, J.A. Zemcov, M. Center for AstroPhysical Surveys National Center for Supercomputing Applications UrbanaIL61801 United States School of Physics and Astronomy Cardiff University CardiffCF24 3YB United Kingdom Fermi National Accelerator Laboratory MS209 P.O. Box 500 BataviaIL60510 United States Kavli Institute for Cosmological Physics University of Chicago 5640 South Ellis Avenue ChicagoIL60637 United States Department of Astronomy and Astrophysics University of Chicago 5640 South Ellis Avenue ChicagoIL60637 United States School of Physics University of Melbourne ParkvilleVIC3010 Australia Department of Astronomy University of Illinois Urbana-Champaign 1002 West Green Street UrbanaIL61801 United States NIST Quantum Devices Group 325 Broadway Mailcode 817.03 BoulderCO80305 United States Department of Physics University of Colorado BoulderCO80309 United States Institut d’Astrophysique de Paris UMR 7095 CNRS & Sorbonne Université 98 bis boulevard Arago Paris75014 France High-Energy Physics Division Argonne National Laboratory 9700 South Cass Avenue. LemontIL60439 United States Kavli Institute for Particle Astrophysics and Cosmology Stanford University 452 Lomita Mall StanfordCA94305 United States Department of Physics Stanford University 382 Via Pueblo Mall StanfordCA94305 United States SLAC National Accelerator Laboratory 2575 Sand Hill Road Menlo ParkCA94025 United States California Institute of Technology PasadenaCA91125 United States Jet Propulsion Laboratory California Institute of Technology PasadenaCA91109 United States Enrico Fermi Institute University of Chicago 5640 South Ellis Avenue ChicagoIL60637 United States Department of Physics University of Chicago 5640 South Ellis Avenue ChicagoIL60637 United States Department of Physics McGill Space Institute McGill University 3600 Rue University MontrealQCH3A 2T8 Canada School of Mathematics Statistics & Computer Science University of KwaZulu-Natal Durban South Africa Unive

We report results from an analysis aimed at detecting the trispectrum of the kinematic Sunyaev-Zel’dovich (kSZ) effect by combining data from the South Pole Telescope (SPT) and Herschel-SPIRE experiments over a 100 deg2 field. The SPT observations combine data from the previous and current surveys, namely SPTpol and SPT-3G, to achieve depths of 4.5, 3, and 16 µK-arcmin in bands centered at 95, 150, and 220 GHz. For SPIRE, we include data from the 600 and 857 GHz bands. We reconstruct the velocity-induced large-scale correlation of the small-scale kSZ signal with a quadratic estimator that uses two cosmic microwave background (CMB) temperature maps, constructed by optimally combining data from all the frequency bands. We reject the null hypothesis of a zero trispectrum at 10.3σ level. However, the measured trispectrum contains contributions from both the kSZ and other undesired components, such as CMB lensing and astrophysical foregrounds, with kSZ being sub-dominant. We use the Agora simulations to estimate the expected signal from CMB lensing and astrophysical foregrounds. After accounting for the contributions from CMB lensing and foreground signals, we do not detect an excess kSZ-only trispectrum and use this non-detection to set constraints on reionization. By applying a prior based on observations of the Gunn-Peterson trough, we obtain an upper limit on the duration of reionization of (formula presented). We find these constraints are fairly robust to foregrounds assumptions. This trispectrum measurement is independent of, but consistent with, Planck’s optical depth measurement. This result is the first constraint on the epoch of reionization using the non-Gaussian nature of the kSZ signal. © 2024, CC BY.

关键词： Kinematics

来源：评论

学校读者我要写书评

暂无评论

Neutrinos from Stored Muons (nuSTORM)

arXiv

引用

arXiv 2022年

作者： Alvarez Ruso, L. Alves, T. Boyd, S. Bross, A. Hobson, P.R. Kyberd, P. Lagrange, J.B. Long, Kenneth Lu, X.-G. Pasternak, J. Pfaff, M. Rogers, C. Bhadra, S. Menary, S. Hartz, M. Tang, J. Mosel, U. Garzelli, M.V. Winter, W. Goswami, S. Chakraborty, K. Agarwalla, S.K. Santopinto, E. Bonesini, M. Stanco, L. Orestano, d. Tortora, L. Mori, Y. Kuno, Y. Sato, A. Chung, M. Filthaut, F. Sobczyk, J.T. Gomez-Cadenas, J.J. Hernando Morata, J.A. Alvarez Ruso, L. Cervera, A. donini, A. Hernandez, P. Lopez Pavon, J. Martín-Albo, J. Mena, O. Novella, P. Sorel, M. Ruber, R. Ahdida, C.C. Bartmann, W. Bauche, J. Calviani, M. Charitonidis, N. Gall, J. Goddard, B. Hessler, C. Kopp, J. Lamont, M. Osborne, J.A. Radicioni, E. de Roeck, A. Velotti, F.M. Blondel, A. Messomo, E.N. Sanchez Nieto, F. Uchida, M.A. Easo, S. Edgecock, R.E. Lagrange, J.B. Murray, W. Rogers, C. Back, J.J. Barker, G. Boyd, S.B. Harrison, P.F. Pascoli, S. Hallsjö, S.-P. Soler, F.J.P. O'Keeffe, H.M. Kormos, L. Nowak, J. Ratoff, P. Andreopoulos, C. McCauley, N. Touramanis, C. Alves, T. Colling, d. dornan, P. dunne, P. Franchini, P. Jonsson, P.M. Jurj, P.B. Kurup, A. Litchfield, P. Long, K. Nonnenmacher, T. Pfaff, M. Pasternak, J. Scott, M. Sedgbeer, J.K. Shorrock, W. Wascko, M.O. di Lodovico, F. Katori, T. Bevan, A. Cremonesi, L. Hobson, P. Nichol, R. Appleby, R. Tygier, S. Lu, X. Wark, d. Weber, A. Smith, P.J. Kyberd, P. Smith, d.R. Brice, S.J. Bross, A.d. Chattopadhay, S. Feher, S. Fields, L. Hanlet, P. Mokhov, N. Morfín, J.G. Neuffer, d. Paley, J. Parke, S. Pavlovic, Z. Popovic, M. Rubinov, P. Shiltzev, V. Huber, P. Mariani, C. Link, J.M. Freemire, B. Liu, A. Kaplan, d.M. Snopok, P. Mishra, S.R. Mahn, K. de Gouvêa, A. Pandey, V. Onel, Y. Winn, d. Tanaka, H.A. Hostert, M. Bogacz, S.A. Cremaldi, L. Summers, d. Mcdonald, K.T. Hanson, G. Palmer, M. Liu, M. Centro Mixto CSIC-UVEG Edificio Institutos Investigación Paterna Apartado 22085 Valencia46071 Spain Physics Department Blackett Laboratory Imperial College London Exhibition Road LondonSW7 2AZ United Kingdom Department of Physics University of Warwick CoventryCV4 7AL United Kingdom Fermilab P.O. Box 500 BataviaIL60510-5011 United States Department of Physics and Astronomy Queen Mary University of London LondonE1 4NS United Kingdom College of Engineering Design and Physical Sciences Brunel University Uxbridge Middlesex UB8 3PH United Kingdom STFC Rutherford Appleton Laboratory Harwell Campus DidcotOX11 0QX United Kingdom James-Franck-Str. 1 GarchingD-85748 Germany Department of Physics and Astronomy York University 4700 Keele Street TorontoONM3J 1P3 Canada TRIUMF 4004 Wesbrook Mall VancouverBCV6T 2A3 Canada Kavli Institute for the Physics and Mathematics of the Universe The University of Tokyo Kashiwa Campus 5-1-5 Kashiwanoha Chiba Kashiwa277-8583 Japan Institute of High Energy Physics Chinese Academy of Sciences Beijing China Justus Liebig Universität Ludwigstraße 23 Gießen35390 Germany II. Institut für Theoretische Physik Universität Hamburg Luruper Chaussee 149 Hamburg22761 Germany Platanenallee 6 Zeuthen15738 Germany Physical Research Laboratory Ahmedabad380009 India Institute of Physics Sainik School Post Sachivalaya Marg Orissa Bhubaneswar751005 India INFN Sezione di Genova Via Dodecaneso Genova33-16146 Italy Sezione INFN Milano Bicocca Dipartimento di Fisica G. Occhialini Milano Italy INFN Sezione di Padova Padova35131 Italy INFN Sezione di Roma Tre Dipartimento di Matematica e Fisica Università Roma Tre Roma Italy 2 Asashiro-Nishi Kumatoricho Osaka Sennan-gun590-0494 Japan Osaka University Graduate School School of Science 1-1 Machikaneyama-cho Osaka Toyonaka560-0043 Japan UNIST Ulsan Korea Republic of Nikhef Amsterdam Netherlands Radboud University Nijmegen Netherlands Institute of T

The 2020 Update of the European Strategy for Particle physics (ESPP) [1] recommended that muon beam R&d should be considered a high-priority future initiative and that a programme of experimentation be developed to determine the neutrino cross-sections required to extract the most physics from the dUNE and Hyper-K long-baseline experiments. The ENUBET [2-4] and nuSTORM [5, 6] collaborations have begun to work within and alongside the CERN physics Beyond Colliders study group [7] and the international Muon Collider collaboration [8] to carry out a joint, five-year R&d programme to deliver a detailed plan for the implementation of an infrastructure in which: • ENUBET and nuSTORM deliver the neutrino cross-section measurement programme identified in the ESPP and allow sensitive searches for physics beyond the Standard Model to be carried out;and in which • A 6d muon ionisation cooling experiment is delivered as part of the technology development programme defined by the international Muon Collider collaboration. This document summarises the status of development of the nuSTORM and 6d cooling experiments and identifies opportunities for collaboration in the development of the initiative outlined above. © 2022, CC BY.

关键词： Charged particles

来源：评论

学校读者我要写书评

暂无评论

A NEW PROPOSAL FOR IdENTIFICATION OF dOUBLE-HIT dIFFUSE LARGE B-CELL LYMphOMA BASEd ON THE PREdOMINANCE OF dOUBLE HITS INVOLVING BCL6 REARRANGEMENT IN TAIWAN

引用

Hematological Oncology 2019年第S2期37卷

作者： Y. Su C. Lee S. Hsieh M. Liu C. Fang C. Chen W. Lee Y. Yen J. Whang-peng T. Chao Hematology/oncology Shuang-Ho Hospital New Taipei Taiwan (Republic of China) Anatomic Pathology Taipei Institute of Pathology Taipei Taiwan (Republic of China) Pathology Shuang-Ho Hospital New Taipei Taiwan (Republic of China) Pathology Wan-Fang Hospital Taipei Taiwan (Republic of China) Pathology Taipei Medical University Hospital Taipei Taiwan (Republic of China) The Ph.D. Program for Cancer Molecular Biology and Drug Discovery College of Medical Science and Technology Taipei Medical University Taipei Taiwan (Republic of China) Taipei Cancer Center Taipei Medical University Taipei Taiwan (Republic of China)

来源：评论

学校读者我要写书评

暂无评论

Author Correction: ZFP36L1 and ZFP36L2 inhibit cell proliferation in a cyclin d-dependent and p53-independent manner

引用

Scientific reports 2019年第1期9卷 17457页

作者： Fat-Moon Suk Chi-Ching Chang Ren-Jye Lin Shyr-Yi Lin Shih-Chen Liu Chia-Feng Jau Yu-Chih Liang Division of Gastroenterology Department of Internal Medicine Wan Fang Hospital Taipei Medical University Taipei Taiwan. Division of Allergy Immunology and Rheumatology Department of Internal Medicine School of Medicine College of Medicine Taipei Medical University Taipei Taiwan. Division of Rheumatology Immunology and Allergy Taipei Medical University Hospital Taipei Taiwan. School of Medical Laboratory Science and Biotechnology College of Medical Science and Technology Taipei Medical University Taipei Taiwan. Department of Primary Care Medicine Taipei Medical University Hospital Taipei Taiwan. Department of General Medicine School of Medicine College of Medicine Taipei Medical University Taipei Taiwan. School of Medical Laboratory Science and Biotechnology College of Medical Science and Technology Taipei Medical University Taipei Taiwan. ycliang@tmu.edu.tw. Traditional Herbal Medicine Research Center Taipei Medical University Hospital Taipei Taiwan. ycliang@tmu.edu.tw. Ph.D. Program in Medical Biotechnology College of Medical Science and Technology Taipei Medical University Taipei Taiwan. ycliang@tmu.edu.tw.

An amendment to this paper has been published and can be accessed via a link at the top of the paper.

关键词：

来源：评论

学校读者我要写书评

暂无评论

Guidelines and definitions for research on epithelial-mesenchymal transition (vol 21, pg 341, 2020)

引用

NATURE REVIEWS MOLECULAR CELL BIOLOGY 2021年第12期22卷 834-834页

作者： Yang, Jing Antin, Parker Berx, Geert Blanpain, Cedric Brabletz, Thomas Bronner, Marianne Campbell, Kyra Cano, Amparo Casanova, Jordi Christofori, Gerhard dedhar, Shoukat derynck, Rik Ford, Heide L. Fuxe, Jonas Garcia de Herreros, Antonio Goodall, Gregory J. Hadjantonakis, Anna-Katerina Huang, Ruby Y. J. Kalcheim, Chaya Kalluri, Raghu Kang, Yibin Khew-Goodall, Yeesim Levine, Herbert Liu, Jinsong Longmore, Gregory d. Mani, Sendurai A. Massague, Joan Mayor, Roberto McClay, david Mostov, Keith E. Newgreen, donald F. Nieto, M. Angela Puisieux, Alain Runyan, Raymond Savagner, Pierre Stanger, Ben Stemmler, Marc P. Takahashi, Yoshiko Takeichi, Masatoshi Theveneau, Eric Thiery, Jean Paul Thompson, Erik W. Weinberg, Robert A. Williams, Elizabeth d. Xing, Jianhua Zhou, Binhua P. Sheng, Guojun Departments of Pharmacology and Pediatrics Moores Cancer Center University of California San Diego La Jolla CA USA Department of Cellular and Molecular Medicine University of Arizona Tucson AZ USA Molecular and Cellular Oncology Lab Department of Biomedical Molecular Biology Ghent University Cancer Research Institute Ghent (CRIG) VIB Center for Inflammation Research Ghent Belgium Laboratory of Stem Cells and Cancer Université Libre de Bruxelles Bruxelles Belgium Department of Experimental Medicine 1 Nikolaus-Fiebiger-Center for Molecular Medicine Friedrich-Alexander-University Erlangen-Nürnberg Erlangen Germany Division of Biology and Biological Engineering California Institute of Technology Pasadena CA USA Department of Biomedical Science and Bateson Centre University of Sheffield Sheffield UK Departamento de Bioquímica Universidad Autónoma de Madrid (UAM) Instituto de Investigaciones Biomédicas ‘Alberto Sols’ (CSIC-UAM) IdiPAZ & Centro de Investigación Biomédica en Red de Cáncer (CIBERONC) Madrid Spain Institute for Research in Biomedicine (IRB Barcelona) Barcelona Institute of Science and Technology/Institut de Biologia Molecular de Barcelona (IBMB-CSIC) Barcelona Spain Department of Biomedicine University of Basel Basel Switzerland Department of Biochemistry and Molecular Biology University of British Columbia and British Columbia Cancer Research Centre Vancouver BC Canada Departments of Cell and Tissue Biology and Anatomy University of California at San Francisco San Francisco CA USA Department of Pharmacology University of Colorado Anschutz Medical Campus Aurora CO USA Department of Laboratory Medicine (LABMED) Division of Pathology Karolinska University Hospital and Department of Microbiology Tumor and Cell Biology (MTC) Karolinska Institutet Stockholm Sweden Programa de Recerca en Càncer Institut Hospital del Mar d’Investigacions Mèdiques (IMIM) and Departament de Ciències Experimentals i de la Salut Universitat Pompeu Fabra Barcelona Spain C

来源：评论

学校读者我要写书评

暂无评论

3d Compressible Navier-Stokes Equations Solve Optical Properties of Forced Shear Layers

引用

Procedia engineering 2017年 174卷 179-187页

作者： Bor-Jang Tsai Yeong-Pei Tsai Chung-Chyi Chou Yu-Tsung Ho Ph.D. Program in Engineering Science Chung Hua University 707 Sec.2 WuFu Rd. Hsinchu 300 Taiwan (ROC) Department of Fire and Safety Da-Yeh University No.168 University Rd. Dacun Changhua 515 Taiwan (ROC) Ding-Hui Project Management Consultants No.424 Dannan Road Taipei 111 Taiwan (ROC)

The optical properties of shear layers is a topic of research with applications in high power lasers and optical imaging systems. In recent years, it has been shown that large-scale structures are intrinsic features in a plane turbulent mixing layer. While there has been some research on the effects of turbulence on laser beams, there has been no study of the optical effects of large-scale structures as they exist in shear layer development, nor how these effects may be controlled. Since the susceptibility of a free shear layer to a forcing input increases as the location of the forcing moves closer to the trailing edge of the splitter plate. disturbances can be imposed on shear layer using very small-amplitude displacements of the splitter-plate trailing edge in a direction perpendicular to the flow direction. We are studying the optical effects of large-scale structures in forced and unforced situations using periodic motion of a small flap at the trailing edge of the splitter plate. Three-dimensional Navier-Stokes equations in conservation law form are solved directly using the WENO scheme for the simulation of a spatially-developing free shear layer.

关键词： MacCormack Method Godunov Method Strehl Ratio

来源：评论

学校读者我要写书评

暂无评论

Native diversity buffers against severity of non-native tree invasions ( vol 621,pg 773 , 2023 )

引用

NATURE 2023年第7982期622卷 E2-E2页

作者： delavaux, Camille S. Crowther, Thomas W. Zohner, Constantin M. Robmann, Niamh M. Lauber, Thomas van den Hoogen, Johan Kuebbing, Sara Liang, Jingjing de-Miguel, Sergio Nabuurs, Gert-Jan Reich, Peter B. Abegg, Meinrad Yao, Yves C. Adou Alberti, Giorgio Zambrano, Angelica M. Almeyda Alvarado, Braulio Vilchez Alvarez-davila, Esteban Alvarez-Loayza, Patricia Alves, Luciana F. Ammer, Christian Anton-Fernandez, Clara Araujo-Murakami, Alejandro Arroyo, Luzmila Avitabile, Valerio Aymard, Gerardo A. Baker, Timothy R. Balazy, Radomir Banki, Olaf Barroso, Jorcely G. Bastian, Meredith L. Bastin, Jean-Francois Birigazzi, Luca Birnbaum, philippe Bitariho, Robert Boeckx, Pascal Bongers, Frans Bouriaud, Olivier Brancalion, Pedro H. S. Brandl, Susanne Brienen, Roel Broadbent, Eben N. Bruelheide, Helge Bussotti, Filippo Gatti, Roberto Cazzolla Cesar, Ricardo G. Cesljar, Goran Chazdon, Robin Chen, Han Y. H. Chisholm, Chelsea Cho, Hyunkook Cienciala, Emil Clark, Connie Clark, david Colletta, Gabriel d. Coomes, david A. Valverde, Fernando Cornejo Corral-Rivas, Jose J. Crim, philip M. Cumming, Jonathan R. dayanandan, Selvadurai de Gasper, Andre L. decuyper, Mathieu derroire, Geraldine deVries, Ben djordjevic, Ilija dolezal, Jiri dourdain, Aurelie Obiang, Nestor Laurier Engone Enquist, Brian J. Eyre, Teresa J. Fandohan, Adande Belarmain Fayle, Tom M. Feldpausch, Ted R. Ferreira, Leandro V. Fischer, Markus Fletcher, Christine Frizzera, Lorenzo Gamarra, Javier G. P. Gianelle, damiano Glick, Henry B. Harris, david J. Hector, Andrew Hemp, Andreas Hengeveld, Geerten Herault, Bruno Herbohn, John L. Herold, Martin Hillers, Annika Coronado, Euridice N. Honorio Hui, Cang Ibanez, Thomas T. Amaral, Ieda Imai, Nobuo Jagodzinski, Andrzej M. Jaroszewicz, Bogdan Johannsen, Vivian Kvist Joly, Carlos A. Jucker, Tommaso Jung, Ilbin Karminov, Viktor Kartawinata, Kuswata Kearsley, Elizabeth Kenfack, david Kennard, deborah K. Kepfer-Rojas, Sebastian Keppel, Gunnar Khan, Mohammed Latif Killeen, Timothy J. Kim, Hyun Seok Kitayama, Kanehiro Kohl, Michael Korju Institute of Integrative Biology ETH Zurich (Swiss Federal Institute of Technology) Zurich Switzerland Department of Genetics Evolution and Environment University College London London UK The Forest School at The Yale School of the Environment Yale University New Haven CT USA Department of Forestry and Natural Resources Purdue University West Lafayette IN USA Department of Agriculture Forestry and Bioresources Seoul National University Seoul South Korea Department of Crop and Forest Sciences University of Lleida Lleida Spain Joint Research Unit CTFC–AGROTECNIO–CERCA Solsona Spain Wageningen University and Research Wageningen The Netherlands World Agroforestry (ICRAF) Nairobi Kenya Department of Forest Resources University of Minnesota St Paul MN USA Hawkesbury Institute for the Environment Western Sydney University Penrith New South Wales Australia Institute for Global Change Biology and School for Environment and Sustainability University of Michigan Ann Arbor MI USA Swiss Federal Institute for Forest Snow and Landscape Research WSL Birmensdorf Switzerland UFR Biosciences University Félix Houphouët-Boigny Abidjan Côte d’Ivoire Department of Agricultural Food Environmental and Animal Sciences University of Udine Udine Italy Faculty of Science and Technology Free University of Bolzano Bolzano Italy Spatial Ecology and Conservation Laboratory Department of Tourism Recreation and Sport Management University of Florida Gainesville FL USA Forestry School Tecnológico de Costa Rica TEC Cartago Costa Rica Fundacion ConVida Universidad Nacional Abierta y a Distancia UNAD Medellin Colombia Field Museum of Natural Histiory Chicago IL USA Center for Tropical Research Institute of the Environment and Sustainability UCLA Los Angeles CA USA Silviculture and Forest Ecology of the Temperate Zones University of Göttingen Göttingen Germany Division of Forest and Forest Resources Norwegian Institute of Bioeconomy Research (NIBIO) Ås Norway Museo de Hi

来源：评论

学校读者我要写书评

暂无评论

建议与咨询留下您的常用邮箱和电话号码，以便我们向您反馈解决方案和替代方法

时间限定

文献类型

馆藏选择

核心期刊

语言

文献类型

帮助

文字说明：

检索规则说明：

检索范例：

分类表

所选分类

限定检索结果

文献类型

馆藏范围

日期分布

学科分类号

主题

机构

作者

语言

请选择保存的检索档案：

请选择收藏分类：

通借通还

建议与咨询 留下您的常用邮箱和电话号码，以便我们向您反馈解决方案和替代方法

时间限定

文献类型

馆藏选择

核心期刊

语言

文献类型

帮助

文字说明：

检索规则说明：

检索范例：

分类表

所选分类

限定检索结果

文献类型

馆藏范围

日期分布

学科分类号

主题

机构

作者

语言

请选择保存的检索档案： 新增检索档案 确定 取消

请选择收藏分类： 新增自定义分类 确定 取消

通借通还

建议与咨询留下您的常用邮箱和电话号码，以便我们向您反馈解决方案和替代方法

请选择保存的检索档案：

请选择收藏分类：