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A search for high-energy neutrinos interacting within the IceCube detector between 2010 and 2012 provided the first evidence for a high-energy neutrino flux of extraterrestrial origin. Results from an analysis using the same methods with a…

High Energy Astrophysical Phenomena · Physics 2016-08-11 M. G. Aartsen , M. Ackermann , J. Adams , J. A. Aguilar , M. Ahlers , M. Ahrens , D. Altmann , T. Anderson , C. Arguelles , T. C. Arlen , J. Auffenberg , X. Bai , S. W. Barwick , V. Baum , J. J. Beatty , J. Becker Tjus , K. -H. Becker , S. BenZvi , P. Berghaus , D. Berley , E. Bernardini , A. Bernhard , D. Z. Besson , G. Binder , D. Bindig , M. Bissok , E. Blaufuss , J. Blumenthal , D. J. Boersma , C. Bohm , D. Bose , S. Böser , O. Botner , L. Brayeur , H. -P. Bretz , A. M. Brown , J. Casey , M. Casier , D. Chirkin , A. Christov , B. Christy , K. Clark , L. Classen , F. Clevermann , S. Coenders , D. F. Cowen , A. H. Cruz Silva , M. Danninger , J. Daughhetee , J. C. Davis , M. Day , J. P. A. M. de André , C. De Clercq , S. De Ridder , P. Desiati , K. D. de Vries , M. de With , T. DeYoung , J. C. Díaz-Vélez , M. Dunkman , R. Eagan , B. Eberhardt , B. Eichmann , J. Eisch , S. Euler , P. A. Evenson , O. Fadiran , A. R. Fazely , A. Fedynitch , J. Feintzeig , J. Felde , T. Feusels , K. Filimonov , C. Finley , T. Fischer-Wasels , S. Flis , A. Franckowiak , K. Frantzen , T. Fuchs , T. K. Gaisser , J. Gallagher , L. Gerhardt , D. Gier , L. Gladstone , T. Glüsenkamp , A. Goldschmidt , G. Golup , J. G. Gonzalez , J. A. Goodman , D. Góra , D. T. Grandmont , D. Grant , P. Gretskov , J. C. Groh , A. Groß , C. Ha , C. Haack , A. Haj Ismail , P. Hallen , A. Hallgren , F. Halzen , K. Hanson , D. Hebecker , D. Heereman , D. Heinen , K. Helbing , R. Hellauer , D. Hellwig , S. Hickford , G. C. Hill , K. D. Hoffman , R. Hoffmann , A. Homeier , K. Hoshina , F. Huang , W. Huelsnitz , P. O. Hulth , K. Hultqvist , S. Hussain , A. Ishihara , E. Jacobi , J. Jacobsen , K. Jagielski , G. S. Japaridze , K. Jero , O. Jlelati , M. Jurkovic , B. Kaminsky , A. Kappes , T. Karg , A. Karle , M. Kauer , J. L. Kelley , A. Kheirandish , J. Kiryluk , J. Kläs , S. R. Klein , J. -H. Köhne , G. Kohnen , H. Kolanoski , A. Koob , L. Köpke , C. Kopper , S. Kopper , D. J. Koskinen , M. Kowalski , A. Kriesten , K. Krings , G. Kroll , J. Kunnen , N. Kurahashi , T. Kuwabara , M. Labare , D. T. Larsen , M. J. Larson , M. Lesiak-Bzdak , M. Leuermann , J. Leute , J. Lünemann , O. Macías , J. Madsen , G. Maggi , R. Maruyama , K. Mase , H. S. Matis , F. McNally , K. Meagher , A. Meli , T. Meures , S. Miarecki , E. Middell , E. Middlemas , N. Milke , J. Miller , L. Mohrmann , T. Montaruli , R. Morse , R. Nahnhauer , U. Naumann , H. Niederhausen , S. C. Nowicki , D. R. Nygren , A. Obertacke , S. Odrowski , A. Olivas , A. Omairat , A. O'Murchadha , T. Palczewski , L. Paul , Ö. Penek , J. A. Pepper , C. Pérez de los Heros , C. Pfendner , D. Pieloth , E. Pinat , J. Posselt , P. B. Price , G. T. Przybylski , J. Pütz , M. Quinnan , L. Rädel , M. Rameez , K. Rawlins , P. Redl , I. Rees , R. Reimann , E. Resconi , W. Rhode , M. Richman , B. Riedel , S. Robertson , J. P. Rodrigues , M. Rongen , C. Rott , T. Ruhe , B. Ruzybayev , D. Ryckbosch , S. M. Saba , H. -G. Sander , M. Santander , S. Sarkar , K. Schatto , F. Scheriau , T. Schmidt , M. Schmitz , S. Schoenen , S. Schöneberg , A. Schönwald , A. Schukraft , L. Schulte , O. Schulz , D. Seckel , Y. Sestayo , S. Seunarine , R. Shanidze , C. Sheremata , M. W. E. Smith , D. Soldin , G. M. Spiczak , C. Spiering , M. Stamatikos , T. Stanev , N. A. Stanisha , A. Stasik , T. Stezelberger , R. G. Stokstad , A. Stößl , E. A. Strahler , R. Ström , N. L. Strotjohann , G. W. Sullivan , H. Taavola , I. Taboada , A. Tamburro , A. Tepe , S. Ter-Antonyan , A. Terliuk , G. Tešić , S. Tilav , P. A. Toale , M. N. Tobin , D. Tosi , M. Tselengidou , E. Unger , M. Usner , S. Vallecorsa , N. van Eijndhoven , J. Vandenbroucke , J. van Santen , M. Vehring , M. Voge , M. Vraeghe , C. Walck , M. Wallraff , Ch. Weaver , M. Wellons , C. Wendt , S. Westerhoff , B. J. Whelan , N. Whitehorn , C. Wichary , K. Wiebe , C. H. Wiebusch , D. R. Williams , H. Wissing , M. Wolf , T. R. Wood , K. Woschnagg , D. L. Xu , X. W. Xu , J. P. Yanez , G. Yodh , S. Yoshida , P. Zarzhitsky , J. Ziemann , S. Zierke , M. Zoll

The most energetic astrophysical sources in the Milky Way, cosmic accelerators capable of producing high-energy cosmic rays, have resisted discovery for over a century. Up to now, astrophysicists sought these sources mainly by scouring the…

High Energy Astrophysical Phenomena · Physics 2023-12-14 Mauricio Bustamante

The comparison of cosmic abundances of the light elements with the density of baryonic stars and gas in the universe today provides a critical test of big bang theory and a powerful probe of the nature of dark matter. A new technique allows…

Astrophysics · Physics 2009-09-25 Craig J. Hogan

Deep elemental composition is a challenging measurement to achieve in the giant planets of the solar system. Yet, knowledge of the deep composition offers important insights in the internal structure of these planets, their evolutionary…

Earth and Planetary Astrophysics · Physics 2024-07-11 Thibault Cavalié , Jonathan Lunine , Olivier Mousis , Ricardo Hueso

By plotting empirical chemical element abundances on Earth relative to the Sun and normalized to silicon versus their first ionization potentials, we confirm the existence of a correlation reported earlier. To explain this, we develop a…

Earth and Planetary Astrophysics · Physics 2022-01-20 Herve Toulhoat , Viacheslav Zgonnik

The discovery ten years ago that the expansion of the Universe is accelerating put in place the last major building block of the present cosmological model, in which the Universe is composed of 4% baryons, 20% dark matter, and 76% dark…

Astrophysics · Physics 2009-02-27 Joshua Frieman , Michael Turner , Dragan Huterer

Hydrogen, the most abundant element in the Universe, has traditionally been used to investigate astrophysical processes within and around our own Galaxy. In its chemically neutral, atomic form (known as HI in the astronomical literature),…

Cosmology and Nongalactic Astrophysics · Physics 2024-11-14 Hamsa Padmanabhan

The outcome of a single quantum experiment is unpredictable, except in a pure-state limit. The definite process that takes place in the apparatus may either be intrinsically random or be explainable from a deeper theory. While the first…

Quantum Physics · Physics 2015-06-22 Theo M. Nieuwenhuizen

Results of experimental studies of electric explosion, in water, of foils made of extremely pure materials are presented. New chemical elements detected both by spectroscopic measurements during the electric discharge and by a…

Plasma Physics · Physics 2007-05-23 L. I. Urutskoev , V. I. Liksonov , V. G. Tsinoev

On the twentieth anniversary of the observation of the top quark, we trace our understanding of this heaviest of all known particles from the prediction of its existence, through the searches and discovery, to the current knowledge of its…

High Energy Physics - Experiment · Physics 2016-03-17 E. Boos , O. Brandt , D. Denisov , S. Denisov , P. Grannis

Since more than a century we investigate cosmic particles coming from the Universe with the aim of understanding their nature, their origin and how they are accelerated. So far, cosmic rays have provided many impressive results, giving…

High Energy Astrophysical Phenomena · Physics 2016-12-30 Mariangela Settimo

In a previous paper we addressed the question "Does the Rapid Appearance of Life on Earth Suggest that Life is Common in the Universe?" The non-observability of recent biogenesis is a self-selection effect that needs to be considered if…

Astrophysics · Physics 2009-11-07 Charles H. Lineweaver , Tamara M. Davis

The heaviest of the transuranic elements known as superheavy elements (SHE) are produced in nuclear reactions in a few specialized laboratories located in Germany, the U.S., Russia, and Japan. The history of this branch of physical science…

History and Philosophy of Physics · Physics 2017-08-15 Helge Kragh

The dark matter problem is almost a century old. Since the 1930s evidence has been growing that our cosmos is dominated by a new form of non-baryonic matter, that holds galaxies and clusters together and influences cosmic structures up to…

Cosmology and Nongalactic Astrophysics · Physics 2018-01-25 Laura Baudis

The article is an historical overview of some of the major contributions from different areas of Science with which, for centuries, it has been built up a scientific, sound and consistent vision of the atom. Some experiments that led us to…

History and Philosophy of Physics · Physics 2021-09-22 Francisco Caruso , Vitor Oguri

Recently it has been proposed that the main contributor to the dark energy of the Universe is a dynamical, slow evolving, spatially inhomogeneous scalar field called quintessence. We investigate the behavior of this scalar field at galactic…

Astrophysics · Physics 2007-05-23 T. Matos , F. S. Guzman

An introductory account is given of the understanding of the structure of the universe. At present the most plausible theory of the origin of the universe is that it formed from the explosion of an extremely hot and dense fireball several…

Astrophysics · Physics 2007-05-23 H. J. Haubold , A. M. Mathai

The recent detection of the ultra-high energy neutrino KM3-230213A by KM3NeT/ARCA marks the first observation of an astrophysical neutrino with energy above 100 PeV, opening a new window to the ultra-high energy Universe. In this…

High Energy Astrophysical Phenomena · Physics 2026-05-11 Per Arne Sevle Myhr

According to quantum theory, randomness is a fundamental property of the universe yet classical physics is mostly deterministic. In this article I show that it is possible for deterministic systems to arise from random ones and discuss the…

Quantum Physics · Physics 2017-03-07 Ian T. Durham

Quantum coherence is a fundamental property of quantum systems, separating quantum from classical physics. Recently, there has been significant interest in the characterization of quantum coherence as a resource, investigating how coherence…