Results 201 to 210 of about 150,323 (230)
Some of the next articles are maybe not open access.
Quark-quark and quark-antiquark potentials
Physical Review D, 1981Suraj N. Gupta, Stanley F. Radford
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Quest for the Origin of Particles and the Universe, 2007
Cosmology is in the midst of a period of revolutionary discovery, propelled by bold ideas from particle physics and by technological advances from gigapixel charge-coupled device cameras to peta-scale computing. The basic features of the universe have now been determined: It is 13.7 billion years old, spatially flat, and expanding at an accelerating ...
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Cosmology is in the midst of a period of revolutionary discovery, propelled by bold ideas from particle physics and by technological advances from gigapixel charge-coupled device cameras to peta-scale computing. The basic features of the universe have now been determined: It is 13.7 billion years old, spatially flat, and expanding at an accelerating ...
openaire +2 more sources
Computing in Science & Engineering, 2004
Over the past 25 years (1979-2004), the theoretical-particle physicists who practice lattice-gauge theory have become some of the most frequent users of supercomputing cycles. Although we've long known that atoms consist of electrons surrounding a nucleus made of nucleons (protons and neutrons), we've recently learned that at a deeper level, the ...
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Over the past 25 years (1979-2004), the theoretical-particle physicists who practice lattice-gauge theory have become some of the most frequent users of supercomputing cycles. Although we've long known that atoms consist of electrons surrounding a nucleus made of nucleons (protons and neutrons), we've recently learned that at a deeper level, the ...
openaire +2 more sources
Nature, 1986
Because nucleons are bound states of quarks, nuclear matter should at sufficiently high density become a quark plasma. Assuming quantum chromodynamics as the basic theory of nuclear forces, it is possible to derive strong-interaction thermodynamics and study the nature of this transition.
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Because nucleons are bound states of quarks, nuclear matter should at sufficiently high density become a quark plasma. Assuming quantum chromodynamics as the basic theory of nuclear forces, it is possible to derive strong-interaction thermodynamics and study the nature of this transition.
openaire +1 more source
Heavy-Quark Diffusion in the Quark–Gluon Plasma
Progress in Particle and Nuclear Physics, 2023Hendrik van Hees, Ralf Rapp
exaly
Quarks at Next-to-Eikonal Accuracy in the CGC: Forward Quark-Nucleus Scattering
Physical Review D, 2021Alina Czajka +2 more
exaly
A4 Modular Flavour Model of Quark Mass Hierarchies Close to the Fixed Point τ = i∞
Journal of High Energy Physics, 2023Serguey Petkov, Morimitsu Tanimoto
exaly
Single Top-Quark Production at the Tevatron and the LHC
Reviews of Modern Physics, 2018Reinhard Schwienhorst, Andrea Giammanco
exaly

