Results 61 to 70 of about 21,978 (196)
Hydromagnesite Precipitation in an Ultramafic‐Hosted Alkaline Lake: Insights From Lake Salda for Jezero Crater, Mars
Journal of Geophysical Research: Planets, Volume 131, Issue 5, May 2026.Abstract
Lake Salda (SW Turkey) is one of the most compelling terrestrial analogs for Jezero Crater on Mars due to its highly alkaline, Mg‐rich waters and hydromagnesite‐forming microbialites. This study integrates hydrochemical measurements, saturation‐index modeling, SEM–TEM imaging, and X‐ray diffraction (XRD) analysis to disentangle the biotic and ...Mirosław Słowakiewicz, Mario Borrelli, Gürçay Kıvanç Akyıldız, Marek Szczerba, Ezher Tagliasacchi, Edoardo Perri +5 morewiley +1 more sourceDark matter annihilation into leptons through gravity portals
Journal of High Energy Physics, 2021 Dark matter (DM) constitutes 85% of the matter in the Universe. However, its specific particle property is still unclear. The fundamentals of DM particles subject to gravitational interaction, and that the lepton excess in cosmic rays may originate from ...Xudong Sun, Ben-Zhong Daidoaj +1 more sourceGravitino dark matter in brane-world cosmology [PDF]
, 2007 The gravitino dark matter hypothesis in the brane cosmology is studied. The
theoretical framework is the CMSSM for particle physics and RS II brane model
for gravity.Aliev A N, Brandenburg A, Brown R A, CDF Collaboration, Cerdeno D G, Covi L, Djouadi A Kneur J L Moultaka G, Edsjo J, Grigoris Panotopoulos, Heinemeyer S, Kiritsis E, Kiritsis E, Kofinas G, Panotopoulos G, Peccei R D, Pradler J Steffen F D, Roszkowski L, Spergel D N, Steffen F D +18 morecore +3 more sourcesRyugu reference project: Recommendations from the measurement definition team
Meteoritics &Planetary Science, Volume 61, Issue 5, Page 819-848, May 2026.Abstract
Sample return missions play a significant role in planetary science by providing pristine extraterrestrial materials. JAXA's Hayabusa2 and NASA's OSIRIS‐REx missions have returned samples from the C‐type asteroids Ryugu and Bennu, respectively. The chemical and mineralogical compositions of these samples closely resemble those of CI chondrites,Tetsuya Yokoyama, Guillaume Avice, Henner Busemann, Nicolas Dauphas, Daniel P. Glavin, Ashley J. King, Thorsten Kleine, Katharina Lodders, Frederic Moynier, Maria Schönbächler, Yoshinori Takano, Kun Wang, Hikaru Yabuta, Yuma Enokido, Ryota Fukai, Shogo Tachibana, Tomohiro Usui +16 morewiley +1 more sourceConstraints on axion-like particles with the Perseus Galaxy Cluster with MAGIC [PDF]
Physics of the Dark UniverseAxion-like particles (ALPs) are pseudo-Nambu-Goldstone bosons that emerge in various theories beyond the standard model. These particles can interact with high-energy photons in external magnetic fields, influencing the observed gamma-ray spectrum.M. Abe, S. Abe, J. Abhir, V. Acciari, I. Agudo, T. Aniello, S. Ansoldi, L. A. Antonelli, A. Engels, C. Arcaro, M. Artero, K. Asano, D. Baack, A. Babi'c, A. Baquero, U. D. Almeida, J. Barrio, I. Batkovi'c, J. Baxter, J. B. Gonz'alez, W. Bednarek, E. Bernardini, J. Bernete, A. Berti, J. Besenrieder, C. Bigongiari, A. Biland, O. Blanch, G. Bonnoli, vZ. Bovsnjak, I. Burelli, G. Busetto, A. Campoy-Ordaz, A. Carosi, R. Carosi, M. Carretero-Castrillo, A. Castro-Tirado, G. Ceribella, Y. Chai, A. Cifuentes, S. Cikota, E. Colombo, J. Contreras, J. Cortina, S. Covino, G. D'Amico, V. D’Elia, P. D. Vela, F. Dazzi, A. D. Angelis, B. Lotto, A. Popolo, J. Delgado, C. Mendez, D. Depaoli, F. Pierro, L. Venere, A. Donini, D. Dorner, M. Doro, D. Elsaesser, G. Emery, J. Escudero, L. Fariña, A. Fattorini, L. Foffano, L. Font, S. Fukami, Y. Fukazawa, R. L'opez, M. Garczarczyk, S. Gasparyan, M. Gaug, J. Paiva, N. Giglietto, F. Giordano, P. Gliwny, N. Godinovi'c, R. Grau, D. Green, J. Green, D. Hadasch, A. Hahn, T. Hassan, L. Heckmann, J. Herrera, D. Hrupec, M. Hutten, R. Imazawa, T. Inada, R. Iotov, K. Ishio, I. Mart'inez, J. Jormanainen, D. Kerszberg, G. Kluge, Y. Kobayashi, P. M. Kouch, H. Kubo, J. Kushida, M. L'ainez, A. Lamastra, F. Leone, E. Lindfors, L. Linhoff, S. Lombardi, F. Longo, R. L'opez-Coto, M. L'opez-Moya, A. L'opez-Oramas, S. Loporchio, A. Lorini, B. Fraga, P. Majumdar, M. Makariev, G. Maneva, N. Mang, M. Manganaro, S. Mangano, K. Mannheim, M. Mariotti, M. Mart'inez, M. Mart'inez-Chicharro, A. Mas-Aguilar, D. Mazin, S. Menchiari, S. Mender, D. Miceli, T. Miener, J. Miranda, R. Mirzoyan, M. Gonz'alez, E. Molina, H. A. Mondal, A. Moralejo, D. Morcuende, T. Nakamori, C. Nanci, L. Nava, V. Neustroev, L. Nickel, M. Rosillo, C. Nigro, L. Nikoli'c, K. Nilsson, K. Nishijima, T. Ekoume, K. Noda, S. Nozaki, Y. Ohtani, A. Okumura, J. Otero-Santos, S. Paiano, M. Palatiello, D. Paneque, R. Paoletti, J. Paredes, D. Pavlovi'c, M. Persic, M. Pihet, G. Pirola, F. Podobnik, P. Moroni, E. Prandini, G. Principe, C. Priyadarshi, W. Rhode, M. Rib'o, J. Rico, C. Righi, N. Sahakyan, T. Saito, K. Satalecka, F. Saturni, B. Schleicher, K. Schmidt, F. Schmuckermaier, J. L. Schubert, T. Schweizer, A. Sciaccaluga, J. Sitarek, V. Sliusar, D. Sobczynska, A. Spolon, A. Stamerra, J. Strivskovi'c, D. Strom, M. Strzys, Y. Suda, S. Suutarinen, H. Tajima, M. Takahashi, R. Takeishi, F. Tavecchio, P. Temnikov, K. Terauchi, T. Terzi'c, M. Teshima, L. Tosti, S. Truzzi, A. Tutone, S. Ubach, J. Scherpenberg, M. Acosta, S. Ventura, V. Verguilov, I. Viale, C. Vigorito, V. Vitale, I. Vovk, R. Walter, M. Will, T. Yamamoto, J. I. F. C. Research, T. U. O. Tokyo, Kashiwa, 277-8582 Chiba, Japan., E. Zurich, CH-8093 Zurich, Switzerland., Instituto de Astrof'isica de Canarias, D. Astrof'isica, U. L. Laguna, E-38200, L. Laguna, Tenerife, Spain., Instituto de Astrof'isica de Andaluc'ia-CSIC, Glorieta de la Astronom'ia sn, 18008, Granada, National Centre for Radio Astrophysics, I-00136 Rome, Italy, U. Udine, I. Trieste, I. Udine, M. F. Physik, D. Garching, Germany, U. Padova, Infn, I-35131 Padova, Institut de F'isica d'Altes Energies, T. Z. F. O. Science, Technology, E-08193 Bellaterra, Technische Universitat Dortmund, D. Dortmund, C. Zagreb, Faculty of Electrical Engineering, Computing, 10000 Zagreb, Croatia., I. Institute, E. Department, U. Madrid, E. Madrid, Centro Brasileiro de Pesquisas F'isicas, 22290-180 Urca, R. Janeiro, Brazil, U. Lodz, F. O. Physics, Applied Informatics, D. O. Astrophysics, 9. Lodz, Poland, Centro de Investigaciones Energ'eticas, Medioambientales y Tecnol'ogicas, Departament de F'isica, CERES-IEEC, U. Barcelona, U. Pisa, I. Pisa, I. Pisa, U. Barcelona, Iccub, IEEC-UB, E. Barcelona, Department for Physics, Universityof Bergen, Norway., I. Catania, D. Astronomia, U. Catania, I. Catania, I. Torino, U. Torino, I. Torino, I. Bari, D. Bari, I. Bari, U. Wurzburg, D-97074 Wurzburg, U. Geneva, 16 Chemind'Ecogia, CH-1290 Versoix, Japanese Magic Group Physics Program, Graduate School of Science, Engineering, H. University, 739-8526 Hiroshima, D. Elektronen-Synchrotron, D. Zeuthen, Armenian Magic Group ICRANet-Armenia, 0019 Yerevan, Armenia, C. Split, M. Engineering, Naval Architecture, 21000 Split, Croatia Croatian Magic Group Josip Juraj Strossmayer Unive Osijek, D. Physics, 31000 Osijek, Finnish Magic Consortium Finnish Centre of Astronomy with Eso, Astronomy, U. Turku, F. Turku, Finland., J. D. O. Physics, T. University, Hiratsuka, 259-1292 Kanagawa, U. Siena, I-53100 Siena, S. S. I. O. Physics, A. C. O. L. P. Institute, Kolkata 700064, West Bengal, India., Inst. for Nucl. Research, Nucl. Energy, B. A. O. Sciences, BG-1784 Sofia, Bulgaria., C. Rijeka, 51000 Rijeka, Yamagata University, Yamagata 990-8560, Finnish Magic Group Space Physics, A. Unit, U. Oulu, F. Oulu, Japanese Magic Group Chiba University, Icehap, 277-8582 Chiba, J. I. F. C. Research, Kobayashi-Maskawa Institute for the Origin of Particles, the Universe, N. University, 464-6801 Nagoya, Kyoto University, 606-8502 Kyoto, I. Perugia, I. Perugia, I. Vergata, I. Roma, K. University, Kobe, Hyogo 658-8501, A. M. C. F. Astrophysics, Romé, also at Port d'Informaci'o Cient'ifica, also at Institute for Astro-, P. Physics, U. Innsbruck, A. Innsbruck, M Austria, A. D. O. Physics, U. Oslo, A. N. D. D. Fisica, U. Trieste, I. Trieste, D-80805 Munchen, also at Inaf Padova +376 moresemanticscholar +1 more sourceGroup theoretic approach to fermion production
Journal of High Energy Physics, 2019 We propose a universal group theoretic description of the fermion production through any type of interaction to scalar or pseudo-scalar. Our group theoretic approach relies on the group SU(2) × U(1), corresponding to the freedom in choosing ...Ui Min, Minho Son, Han Gyeol Suhdoaj +1 more source