Results 281 to 290 of about 1,963,432 (340)

Magnetized plasma rotator for relativistic mid-infrared pulses via frequency-variable Faraday rotation. [PDF]

Light Sci Appl
Li DA, Zhang GB, Pegoraro F, Zhao Q, Liu WJ, Zhu XL, Zou DB, Li JX, Pukhov A, Sheng ZM, Yu TP.   +10 more
europepmc   +1 more source

Alfvén Waves in Partially Ionised Solar Steady-State Plasmas. [PDF]

Sol Phys
Alshehri NF, Ballai I, Verth G, Fedun V.
europepmc   +1 more source

A comparative study of target fabrication strategies for microgram muonic atom spectroscopy. [PDF]

Sci Rep
Antwis L, Bara S, Bruhn C, Cocolios TE, Deseyn M, Doinaki A, Düllmann CE, Fletcher J, Heines M, Heller R, Indelicato P, Kentsch U, Kieck T, Kirch K, Knecht A, Maugeri EA, Niikura M, Ouf A, Pereira LMC, Phyo WWMM, Pohl R, Renisch D, Ritjoho N, Vantomme A, Vogiatzi SM, von Schoeler K, Wauters F, Zendour A, Zweidler S.   +28 more
europepmc   +1 more source

Achieving GPT-4o level performance in astronomy with a specialized 8B-parameter large language model. [PDF]

Sci Rep
de Haan T, Ting YS, Ghosal T, Nguyen TD, Accomazzi A, Wells A, Ramachandra N, Pan R, Sun Z.   +8 more
europepmc   +1 more source

Black Holes as Laboratories: Tests of General Relativity. [PDF]

Gen Relativ Gravit
Gregory R, Nissanke S.
europepmc   +1 more source

Observation of sub-relativistic collisionless shock generation and breakout dynamics. [PDF]

Nat Commun
Bai Y, Zhang D, Zeng Y, Mao J, Song L, Tian Y, Li R.   +6 more
europepmc   +1 more source

GSI-ESA-NASA Nuclear Cross-section Database: Update II. Elemental and Isotopic Fragment-production Cross Sections. [PDF]

Health Phys
Luoni F, Szabo R, de Wet W, Norman R, Werneth C.   +4 more
europepmc   +1 more source

Galaxy Tomography with the Gravitational Wave Background from Supermassive Black Hole Binaries

Chen Y.
europepmc   +1 more source

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High-energy neutrino astrophysics

Nature Physics, 2016
The chargeless, weakly interacting neutrinos are ideal astronomical messengers as they travel through space without scattering, absorption or deflection. But this weak interaction also makes them notoriously difficult to detect, leading to neutrino observatories requiring large-scale detectors.
F. Halzen
openaire   +2 more sources