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Taux d'acceptation attendu 80%
Detection of the large-scale tidal field with galaxy multiplet alignment in the DESI Y1 spectroscopic survey
T. Physics
Claire Lamman ,
1★ Daniel Eisenstein,1
Jaime E. Forero-Romero ,
2,3
Jessica Nicole Aguilar,4
Steven Ahlen ,
5 Stephen Bailey ,
4 Davide Bianchi ,
6 David Brooks,7 Todd Claybaugh,4
Axel de la Macorra ,
8 Peter Doel,7 Simone Ferraro ,
4,9 Andreu Font-Ribera ,
7,10 Enrique Gaztañaga,11,12,13 Satya Gontcho A Gontcho ,
4 Gaston Gutierrez,14 Klaus Honscheid,15,16,17
Cullan Howlett ,
18 Anthony Kremin ,
4 Andrew Lambert,4 Martin Landriau ,
4 Laurent Le Guillou ,
19
Michael E. Levi ,
4 Aaron Meisner ,
20 Ramon Miquel,21,10 John Moustakas ,
22 Jeffrey A. Newman ,
23
Gustavo Niz ,
24,25 Francisco Prada ,
26 Ignasi Pérez-Ràfols ,
27 Ashley J. Ross ,
15,28,17
Graziano Rossi,29 Eusebio Sanchez ,
30 Michael Schubnell,31,32 David Sprayberry,20 Gregory Tarlé ,
32
Mariana Vargas-Magaña ,
8 Benjamin Alan Weaver,20 Hu Zou 33
Observations and detectability of young Suns’ flaring and CME activity in optical spectra
T. Physics
M. Leitzinger,1⋆ P. Odert,1 R. Greimel2
1 Institute of Physics, Department for Astrophysics and Geophysics, University of Graz, Universitätsplatz 5, 8010 Graz, Austria
1 RG Science, Schanzelgasse 17, 8010 Graz, Austria
Non-Hermitian unidirectional routing of photonic qubits
En-Ze Li,1, 2, ∗ Yi-Yang Liu,3, ∗ Ming-Xin Dong,1, 2 Dong-Sheng Ding,1, 2, 4, † and Bao-Sen Shi1, 2, 4, ‡
1Key Laboratory of Quantum Information, University of Science and Technology of China, Hefei, Anhui 230026, China.
2Synergetic Innovation Center of Quantum Information and Quantum Physics,
University of Science and Technology of China, Hefei, Anhui 230026, China.
3School of Physical Science and Technology, Lanzhou University, Lanzhou, Gansu 730000, China.
4Hefei National Laboratory, Hefei, Anhui, 230088, China
Electronic and thermal sequential transport in metallic and superconducting two-junction arrays
T. Physics
T. K¨uhn
NanoScience Center and Department of Physics, University of Jyv¨askyl¨a,
P.O. Box 35 (YFL), FIN-40014 University of Jyv¨askyl¨a, Finland
G. S. Paraoanu∗
Low Temperature Laboratory, School of Science and Technology,
Aalto University, P. O. Box 15100, FI-00076 AALTO, Finland.
Probing supermassive black hole seed scenarios with gravitational wave measurements
Astrophysics
John Ellis,1, 2, 3, ∗ Malcolm Fairbairn,1, † Juan Urrutia,3, 4, ‡ and Ville Vaskonen3, 5, 6, §
1King’s College London, Strand, London, WC2R 2LS, United Kingdom
2Theoretical Physics Department, CERN, Geneva, Switzerland
3Keemilise ja Bioloogilise F¨u¨usika Instituut, R¨avala pst. 10, 10143 Tallinn, Estonia
4Department of Cybernetics, Tallinn University of Technology, Akadeemia tee 21, 12618 Tallinn, Estonia
5Dipartimento di Fisica e Astronomia, Universit`a degli Studi di Padova, Via Marzolo 8, 35131 Padova, Italy
6Istituto Nazionale di Fisica Nucleare, Sezione di Padova, Via Marzolo 8, 35131 Padova, Italy
Protoplanetary disks in Ks-band total intensity and polarized light
Exp. Astrophysics
Bin B. Ren (任彬) iD ⋆⋆1, 2, 3
Myriam Benisty iD 1, 2
Christian Ginski iD 4
Ryo Tazaki iD 2
Nicole L. Wallack iD 5
Julien
Milli iD 2
Antonio Garufi iD 6
Jaehan Bae iD 7
Stefano Facchini iD 8
François Ménard iD 2
Paola Pinilla iD 9
C. Swastik iD 10, Richard Teague iD 11, and Zahed Wahhaj iD 12
_________________________________________________________________
1 Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange, Bd de l’Observatoire, CS 34229, 06304
Nice cedex 4, France; bin.ren@oca.eu
2 Université Grenoble Alpes, CNRS, Institut de Planétologie et d’Astrophysique (IPAG), F-38000 Grenoble, France
3 Department of Astronomy, California Institute of Technology, MC 249-17, 1200 E California Blvd, Pasadena, CA 91125, USA
4 School of Natural Sciences, University of Galway, University Road, H91 TK33 Galway, Ireland
5 Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC 20015, USA
6
INAF, Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I-50125 Firenze, Italy
7 Department of Astronomy, University of Florida, Gainesville, FL 32611, USA
8 Dipartimento di Fisica, Universitá degli Studi di Milano, via Celoria 16, I-20133 Milano, Italy
9 Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK
10 Indian Institute of Astrophysics, Koramangala 2nd Block, Bangalore 560034, India
11 Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
12 European Southern Observatory, Alonso de Córdova 3107, Vitacura Casilla 19001, Santiago, Chile
Searching for H→hh→bb¯ττ in the 2HDM Type-I at the LHC
Astrophysics Experimental
A. Arhrib1,2∗
S. Moretti3,4†
S. Semlali3,5‡
C. H. Shepherd-Themistocleous5§
Y. Wang6,7¶, Q. S. Yan8,9‖
------------------------------------------------------
1 Abdelmalek Essaadi University, Faculty of Sciences and Techniques, B.P. 2117 T´etouan,
Tanger, Morocco.
2 Department of Physics and Center for Theory and Computation, National Tsing Hua
University, Hsinchu, Taiwan 300.
3School of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ,
United Kingdom.
4Department of Physics and Astronomy, Uppsala University, Box 516, SE-751 20 Uppsala, Sweden.
5Particle Physics Department, Rutherford Appleton Laboratory, Chilton, Didcot, Oxon OX11 0QX,
United Kingdom.
6College of Physics and Electronic Information, Inner Mongolia Normal University,
Hohhot 010022, PR China.
7
Inner Mongolia Key Laboratory for Physics and Chemistry of Functional Materials,
Inner Mongolia Normal University, Hohhot, 010022, China.
8Center for Future High Energy Physics, Chinese Academy of Sciences,
Beijing 100049, P.R. China.
9School of Physics Sciences, University of Chinese Academy of Sciences,
Beijing 100039, P.R. China.
Surface-Enhanced Raman Scattering from Au Nanorods, Nanotriangles, and Nanostars with Tuned Plasmon Resonances
NanoPhysics
Boris N. Khlebtsov,1
Andrey M. Burov,1 Sergey V. Zarkov,1
Nikolai G. Khlebtsov,1,2,*
----------------------------------------------------
1 Institute of Biochemistry and Physiology of Plants and Microorganisms, "Saratov Scientific
Centre of the Russian Academy of Sciences," 13 Prospekt Entuziastov, Saratov 410049, Russia
2 Saratov State University, 83 Ulitsa Astrakhanskaya, Saratov 410012, Russia
Grating design methodology for tailored free-space beam-forming
ApplScience
Gillenhaal J. Beck,
Jonathan P. Home,
Karan K. Mehta
---------
G.J. Beck and J.P. Home are with the Institute of Quantum Electronics,
ETH Zurich, Zurich, Switzerland. K.K. Mehta is with the school of Electrical
and Computer Engineering, Cornell University, Ithaca, NY, USA. email:
On-demand Generation of Indistinguishable Photons in the Telecom C-Band using Quantum Dot Devices
ApplScience
Daniel A. Vajner,1
Paweł Holewa,2, 3, 4
Emilia Zięba-Ostój,2
Maja Wasiluk,2
Martin von Helversen,1
Aurimas Sakanas,3
Alexander Huck,5
Kresten Yvind,3, 4
Niels Gregersen,3
Anna Musiał,2
Marcin Syperek,2
Elizaveta Semenova,3, 4
Tobias Heindel1
------
1)Institute of Solid State Physics, Technical University of Berlin, 10623 Berlin, Germany
2)Department of Experimental Physics, Faculty of Fundamental Problems of Technology,
Wrocław University of Science and Technology, Wyb. Wyspia´nskiego 27, 50-370 Wrocław,
Poland
3)DTU Electro, Department of Electrical and Photonics Engineering, Technical University of Denmark, Kongens Lyngby 2800,
Denmark
4)NanoPhoton-Center for Nanophotonics, Technical University of Denmark, 2800 Kongens Lyngby,
Denmark
5)Center for Macroscopic Quantum States (bigQ), Department of Physics, Technical University of Denmark, 2800 Kgs. Lyngby,
Denmark
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