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The Pierre Auger Collaboration discovered, in a solid angle of radius about 18\degree, a local group of cosmic rays having energies in the region E0 \geq 5.5\times1019 eV and coming from the region of the Gen A radio galaxy, whose galactic…

High Energy Astrophysical Phenomena · Physics 2015-06-04 A. V. Glushkov

Spherical harmonic moments are well-suited for capturing anisotropy at any scale in the flux of cosmic rays. An unambiguous measurement of the full set of spherical harmonic coefficients requires full-sky coverage. This can be achieved by…

High Energy Astrophysical Phenomena · Physics 2014-10-09 The Pierre Auger , Telescope Array Collaborations , : , A. Aab , P. Abreu , M. Aglietta , E. J. Ahn , I. Al Samarai , I. F. M. Albuquerque , I. Allekotte , J. Allen , P. Allison , A. Almela , J. Alvarez Castillo , J. Alvarez-Muñiz , R. Alves Batista , M. Ambrosio , A. Aminaei , L. Anchordoqui , S. Andringa , C. Aramo , F. Arqueros , H. Asorey , P. Assis , J. Aublin , M. Ave , M. Avenier , G. Avila , A. M. Badescu , K. B. Barber , J. Bäuml , C. Baus , J. J. Beatty , K. H. Becker , J. A. Bellido , C. Berat , X. Bertou , P. L. Biermann , P. Billoir , M. Blanco , C. Bleve , H. Blümer , M. Boháčová , D. Boncioli , C. Bonifazi , R. Bonino , N. Borodai , J. Brack , I. Brancus , P. Brogueira , W. C. Brown , P. Buchholz , A. Bueno , S. Buitink , M. Buscemi , K. S. Caballero-Mora , B. Caccianiga , L. Caccianiga , M. Candusso , L. Caramete , R. Caruso , A. Castellina , G. Cataldi , L. Cazon , R. Cester , A. G. Chavez , A. Chiavassa , J. A. Chinellato , J. Chudoba , M. Cilmo , R. W. Clay , G. Cocciolo , R. Colalillo , A. Coleman , L. Collica , M. R. Coluccia , R. Conceição , F. Contreras , M. J. Cooper , A. Cordier , S. Coutu , C. E. Covault , J. Cronin , A. Curutiu , R. Dallier , B. Daniel , S. Dasso , K. Daumiller , B. R. Dawson , R. M. de Almeida , M. De Domenico , S. J. de Jong , J. R. T. de Mello Neto , I. De Mitri , J. de Oliveira , V. de Souza , L. del Peral , O. Deligny , H. Dembinski , N. Dhital , C. Di Giulio , A. Di Matteo , J. C. Diaz , M. L. Díaz Castro , F. Diogo , C. Dobrigkeit , W. Docters , J. C. D'Olivo , A. Dorofeev , Q. Dorosti Hasankiadeh , M. T. Dova , J. Ebr , R. Engel , M. Erdmann , M. Erfani , C. O. Escobar , J. Espadanal , A. Etchegoyen , P. Facal San Luis , H. Falcke , K. Fang , G. Farrar , A. C. Fauth , N. Fazzini , A. P. Ferguson , M. Fernandes , B. Fick , J. M. Figueira , A. Filevich , A. Filipčič , B. D. Fox , O. Fratu , U. Fröhlich , B. Fuchs , T. Fuji , R. Gaior , B. García , S. T. Garcia Roca , D. Garcia-Gamez , D. Garcia-Pinto , G. Garilli , A. Gascon Bravo , F. Gate , H. Gemmeke , P. L. Ghia , U. Giaccari , M. Giammarchi , M. Giller , C. Glaser , H. Glass , M. Gómez Berisso , P. F. Gómez Vitale , P. Gonçalves , J. G. Gonzalez , N. González , B. Gookin , A. Gorgi , P. Gorham , P. Gouffon , S. Grebe , N. Griffith , A. F. Grillo , T. D. Grubb , Y. Guardincerri , F. Guarino , G. P. Guedes , M. R. Hampel , P. Hansen , D. Harari , T. A. Harrison , S. Hartmann , J. L. Harton , A. Haungs , T. Hebbeker , D. Heck , P. Heimann , A. E. Herve , G. C. Hill , C. Hojvat , N. Hollon , E. Holt , P. Homola , J. R. Hörandel , P. Horvath , M. Hrabovský , D. Huber , T. Huege , A. Insolia , P. G. Isar , K. Islo , I. Jandt , S. Jansen , C. Jarne , M. Josebachuili , A. Kääpä , O. Kambeitz , K. H. Kampert , P. Kasper , I. Katkov , B. Kégl , B. Keilhauer , A. Keivani , E. Kemp , R. M. Kieckhafer , H. O. Klages , M. Kleifges , J. Kleinfeller , R. Krause , N. Krohm , O. Krömer , D. Kruppke-Hansen , D. Kuempel , N. Kunka , G. La Rosa , D. LaHurd , L. Latronico , R. Lauer , M. Lauscher , P. Lautridou , S. Le Coz , M. S. A. B. Leão , D. Lebrun , P. Lebrun , M. A. Leigui de Oliveira , A. Letessier-Selvon , I. Lhenry-Yvon , K. Link , R. López , A. Lopez Agüera , K. Louedec , J. Lozano Bahilo , L. Lu , A. Lucero , M. Ludwig , M. C. Maccarone , M. Malacari , S. Maldera , M. Mallamaci , J. Maller , D. Mandat , P. Mantsch , A. G. Mariazzi , V. Marin , I. C. Mariş , G. Marsella , D. Martello , L. Martin , H. Martinez , O. Martínez Bravo , D. Martraire , J. J. Masías Meza , H. J. Mathes , S. Mathys , J. A. J. Matthews , J. Matthews , G. Matthiae , D. Maurel , D. Maurizio , E. Mayotte , P. O. Mazur , C. Medina , G. Medina-Tanco , M. Melissas , D. Melo , E. Menichetti , A. Menshikov , S. Messina , R. Meyhandan , S. Mićanović , M. I. Micheletti , L. Middendorf , I. A. Minaya , L. Miramonti , B. Mitrica , L. Molina-Bueno , S. Mollerach , M. Monasor , D. Monnier Ragaigne , F. Montanet , C. Morello , M. Mostafá , C. A. Moura , M. A. Muller , G. Müller , M. Münchmeyer , R. Mussa , G. Navarra , S. Navas , P. Necesal , L. Nellen , A. Nelles , J. Neuser , M. Niechciol , L. Niemietz , T. Niggemann , D. Nitz , D. Nosek , V. Novotny , L. Nožka , L. Ochilo , A. Olinto , M. Oliveira , N. Pacheco , D. Pakk Selmi-Dei , M. Palatka , J. Pallotta , N. Palmieri , P. Papenbreer , G. Parente , A. Parra , T. Paul , M. Pech , J. Pekala , R. Pelayo , I. M. Pepe , L. Perrone , R. Pesce , E. Petermann , C. Peters , S. Petrera , A. Petrolini , Y. Petrov , J. Phuntsok , R. Piegaia , T. Pierog , P. Pieroni , M. Pimenta , V. Pirronello , M. Platino , M. Plum , A. Porcelli , C. Porowski , R. R. Prado , P. Privitera , M. Prouza , V. Purrello , E. J. Quel , S. Querchfeld , S. Quinn , J. Rautenberg , O. Ravel , D. Ravignani , B. Revenu , J. Ridky , S. Riggi , M. Risse , P. Ristori , V. Rizi , J. Roberts , W. Rodrigues de Carvalho , I. Rodriguez Cabo , G. Rodriguez Fernandez , J. Rodriguez Rojo , M. D. Rodríguez-Frías , G. Ros , J. Rosado , T. Rossler , M. Roth , E. Roulet , A. C. Rovero , S. J. Saffi , A. Saftoiu , F. Salamida , H. Salazar , A. Saleh , F. Salesa Greus , G. Salina , F. Sánchez , P. Sanchez-Lucas , C. E. Santo , E. Santos , E. M. Santos , F. Sarazin , B. Sarkar , R. Sarmento , R. Sato , N. Scharf , V. Scherini , H. Schieler , P. Schiffer , O. Scholten , H. Schoorlemmer , P. Schovánek , A. Schulz , J. Schulz , J. Schumacher , S. J. Sciutto , A. Segreto , M. Settimo , A. Shadkam , R. C. Shellard , I. Sidelnik , G. Sigl , O. Sima , A. Śmiał , R. Šmída , G. R. Snow , P. Sommers , J. Sorokin , R. Squartini , Y. N. Srivastava , S. Stanič , J. Stapleton , J. Stasielak , M. Stephan , A. Stutz , F. Suarez , T. Suomijärvi , A. D. Supanitsky , M. S. Sutherland , J. Swain , Z. Szadkowski , M. Szuba , O. A. Taborda , A. Tapia , M. Tartare , V. M. Theodoro , C. Timmermans , C. J. Todero Peixoto , G. Toma , L. Tomankova , B. Tomé , A. Tonachini , G. Torralba Elipe , D. Torres Machado , P. Travnicek , E. Trovato , M. Tueros , R. Ulrich , M. Unger , M. Urban , J. F. Valdés Galicia , I. Valiño , L. Valore , G. van Aar , A. M. van den Berg , S. van Velzen , A. van Vliet , E. Varela , B. Vargas Cárdenas , G. Varner , J. R. Vázquez , R. A. Vázquez , D. Veberič , V. Verzi , J. Vicha , M. Videla , L. Villaseñor , B. Vlcek , S. Vorobiov , H. Wahlberg , O. Wainberg , D. Walz , A. A. Watson , M. Weber , K. Weidenhaupt , A. Weindl , F. Werner , A. Widom , L. Wiencke , B. Wilczyńska , H. Wilczyński , M. Will , C. Williams , T. Winchen , D. Wittkowski , B. Wundheiler , S. Wykes , T. Yamamoto , T. Yapici , P. Younk , G. Yuan , A. Yushkov , B. Zamorano , E. Zas , D. Zavrtanik , M. Zavrtanik , I. Zaw , A. Zepeda , J. Zhou , Y. Zhu , M. Zimbres Silva , M. Ziolkowski , R. U. Abbasi , M. Abe , T. Abu-Zayyad , M. Allen , R. Anderson , R. Azuma , E. Barcikowski , J. W. Belz , D. R. Bergman , S. A. Blake , R. Cady , M. J. Chae , B. G. Cheon , J. Chiba , M. Chikawa , W. R. Cho , T. Fujii , M. Fukushima , T. Goto , W. Hanlon , Y. Hayashi , N. Hayashida , K. Hibino , K. Honda , D. Ikeda , N. Inoue , T. Ishii , R. Ishimori , H. Ito , D. Ivanov , C. C. H. Jui , K. Kadota , F. Kakimoto , O. Kalashev , K. Kasahara , H. Kawai , S. Kawakami , S. Kawana , K. Kawata , E. Kido , H. B. Kim , J. H. Kim , J. H. Kim , S. Kitamura , Y. Kitamura , V. Kuzmin , Y. J. Kwon , J. Lan , S. I. Lim , J. P. Lundquist , K. Machida , K. Martens , T. Matsuda , T. Matsuyama , J. N. Matthews , M. Minamino , K. Mukai , I. Myers , K. Nagasawa , S. Nagataki , T. Nakamura , T. Nonaka , A. Nozato , S. Ogio , J. Ogura , M. Ohnishi , H. Ohoka , K. Oki , T. Okuda , M. Ono , A. Oshima , S. Ozawa , I. H. Park , M. S. Pshirkov , D. C. Rodriguez , G. Rubtsov , D. Ryu , H. Sagawa , N. Sakurai , A. L. Sampson , L. M. Scott , P. D. Shah , F. Shibata , T. Shibata , H. Shimodaira , B. K. Shin , J. D. Smith , P. Sokolsky , R. W. Springer , B. T. Stokes , S. R. Stratton , T. A. Stroman , T. Suzawa , M. Takamura , M. Takeda , R. Takeishi , A. Taketa , M. Takita , Y. Tameda , H. Tanaka , K. Tanaka , M. Tanaka , S. B. Thomas , G. B. Thomson , P. Tinyakov , I. Tkachev , H. Tokuno , T. Tomida , S. Troitsky , Y. Tsunesada , K. Tsutsumi , Y. Uchihori , S. Udo , F. Urban , G. Vasiloff , T. Wong , R. Yamane , H. Yamaoka , K. Yamazaki , J. Yang , K. Yashiro , Y. Yoneda , S. Yoshida , H. Yoshii , R. Zollinger , Z. Zundel

The 2dF Galaxy Redshift Survey is the first to observe more than 100,000 redshifts, making possible precise measurements of many aspects of galaxy clustering. The spatial distribution of galaxies can be studied as a function of galaxy…

Astrophysics · Physics 2009-11-07 J. A. Peacock

Cosmological implications of the observed large-scale peculiar velocities are reviewed, alone or combined with redshift surveys and CMB data. The latest version of the POTENT method for reconstructing the underlying three-dimensional…

Astrophysics · Physics 2007-05-23 Avishai Dekel

Recent combined analyses of the CMB and galaxy cluster data reveal unexpectedly large and anisotropic peculiar velocity fields at large scales. We study cosmic models with included vorticity, acceleration and total angular momentum of the…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-18 Davor Palle

In this paper we consider dynamical behavior of astrophysical objects (galaxies and dwarf galaxies) taking into account both gravitational attraction between them and cosmological expansion of the Universe. First, we obtain the general…

Cosmology and Nongalactic Astrophysics · Physics 2013-04-05 Maxim Eingorn , Alexandra Kudinova , Alexander Zhuk

We explore the scenario that the observable universe emerged from the vicinity of a negative mass ring singularity, and all content of the universe travels at the same group velocity close to the speed of light on a geodesic trajectory…

General Relativity and Quantum Cosmology · Physics 2025-07-03 Michael Zlotnikov

A metric-field approach to gravitation is presented. It is based on an idea of dependency of space-time properties on measuring instruments. Some bimetric equations that realize this idea are considered. They were tested by the binary…

General Relativity and Quantum Cosmology · Physics 2009-11-07 L. V. Verozub

Recent studies suggest that the anisotropy in cosmic-ray arrival directions can provide insight into local acceleration sites and propagation conditions. We developed a unified framework to interpret both the observed energy spectra and the…

High Energy Astrophysical Phenomena · Physics 2025-11-25 Bing-qiang Qiao , Wei Liu , Huirong Yan , Yi-qing Guo

The Galaxy's stellar halo seems to be a tangle of disrupted systems that have been tidally stretched out into streams. Each stream approximately delineates an orbit in the Galactic force-field. In the first paper in this series we showed…

Astrophysics of Galaxies · Physics 2009-10-24 Andy Eyre , James Binney

The meaning of "linear expansion" is explained. Particularly accurate relative distances are compiled and homogenized a) for 246 SNe Ia and 35 clusters with v<30,000 km/s, and b) for relatively nearby galaxies with 176 TRGB and 30 Cepheid…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-13 A. Sandage , B. Reindl , G. A. Tammann

The theory for the selection of the initial state of the universe from the landscape multiverse predicts superhorizon inhomogeneities induced by nonlocal entanglement of our Hubble volume with modes and domains beyond the horizon. Here we…

High Energy Physics - Theory · Physics 2009-02-09 L. Mersini-Houghton , R. Holman

We continue the study of dipole cosmology framework put forward in \cite{Krishnan:2022qbv}, a beyond FLRW setting that has a preferred direction in the metric which may be associated with a cosmological tilt, a cosmic dipole. In this setup…

Cosmology and Nongalactic Astrophysics · Physics 2025-02-11 A. Allahyari , E. Ebrahimian , R. Mondol , M. M. Sheikh-Jabbari

The astronomical observations indicate that the universe expands with acceleration and it has a finite event horizon. The recent CMB observations confirm the universe is homogeneous, isotropic and asymptotically flat. The total…

General Physics · Physics 2014-11-18 Dimitar Valev

We discuss a consistent theory for a self-interacting vector field, breaking an Abelian symmetry in such a way to obtain an interesting behavior for its longitudinal polarization. In an appropriate decoupling limit, the dynamics of the…

High Energy Physics - Theory · Physics 2015-06-18 Gianmassimo Tasinato

We explore potential strategies for testing General Relativity via the coherent motions of galaxies. Our position at z=0 provides the reference point for distance measures in cosmology. By contrast, the Cosmic Microwave Background at z ~…

Cosmology and Nongalactic Astrophysics · Physics 2010-04-06 Fergus Simpson

In the concordance model of the Universe, the matter distribution - as observed in galaxy number counts or the intensity of line emission (such as the 21cm line of neutral hydrogen) - should have a kinematic dipole due to the Sun's motion…

Cosmology and Nongalactic Astrophysics · Physics 2018-01-19 Roy Maartens , Chris Clarkson , Song Chen

The influence of fluctuating conductivity on the coefficients known from the mean-field electrodynamics is considered. If the conductivity fluctuations are assumed as uncorrelated with the turbulent velocity field then only the effective…

Plasma Physics · Physics 2020-07-15 G. Rüdiger , M. Küker , P. J. Käpylä

Objects falling into an overdensity appear larger on its near side and smaller on its far side than other objects at the same redshift. This produces a dipolar pattern of magnification, primarily as a consequence of the Doppler effect. At…

Cosmology and Nongalactic Astrophysics · Physics 2017-10-09 Camille Bonvin , Sambatra Andrianomena , David Bacon , Chris Clarkson , Roy Maartens , Teboho Moloi , Philip Bull

We present the result of a decomposition of the 2dFGRS galaxy overdensity field into an orthonormal basis of spherical harmonics and spherical Bessel functions. Galaxies are expected to directly follow the bulk motion of the density field…

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