Results 61 to 70 of about 164,628 (263)

Octet baryon magnetic moments at next-to-next-to-leading order in covariant chiral perturbation theory

open access: yesEuropean Physical Journal C: Particles and Fields, 2018
We calculate the octet baryon magnetic moments in covariant baryon chiral perturbation theory with the extended-on-mass-shell renormalization scheme up to next-to-next-to-leading order.
Yang Xiao   +4 more
doaj   +1 more source

On the Baryon Fractions in Clusters and Groups of Galaxies [PDF]

open access: yes, 2010
We present the baryon fractions of 2MASS groups and clusters as a function of cluster richness using total and gas masses measured from stacked ROSAT X-ray data and stellar masses estimated from the infrared galaxy catalogs. We detect X-ray emission even
Anderson   +50 more
core   +1 more source

A Brief, Biased View of Neutron Star Cooling

open access: yesAstronomische Nachrichten, Volume 346, Issue 1, January 2025.
ABSTRACT This is a concise and non‐technical review of topics related to neutron star (NS) cooling, for both young NSs and NSs in low‐mass x‐ray binaries. Neutrino emission from the NS core drives cooling rates, via different processes including Urca processes and pair breaking and formation at the neutron superfluid critical temperature.
Craig Heinke
wiley   +1 more source

Baryon decays to purely baryonic final states [PDF]

open access: yesScientific Reports, 2019
AbstractThe LHCb collaboration has presented first experimental evidence that spin-carrying matter and antimatter differ. The study looked at four-body decays of the $${{\boldsymbol{\Lambda }}}_{{\boldsymbol{b}}}^{{\bf{0}}}$$ Λ
Y. K. Hsiao   +3 more
openaire   +5 more sources

Effects of hyperfine interactions on masses of N and Δ baryons

open access: yesIranian Journal of Physics Research, 2009
Presenting a model for theoretical study of baryon masses, either in relativistic or nonrelativistic area, has always been of great importance and several suggestions have been proposed.
H Hassanabadi, S Zarrinkamar, AA Rajabi
doaj  

Radial excitations of the decuplet baryons

open access: yesEuropean Physical Journal C: Particles and Fields, 2017
The ground and first excited states of the decuplet baryons are studied using the two-point QCD sum rule approach. The mass and residue of these states are computed and compared with the existing experimental data and other theoretical predictions.
T. M. Aliev, K. Azizi, H. Sundu
doaj   +1 more source

Baryons and baryonic matter in the large Nc and heavy quark limits [PDF]

open access: yesPhys.Rev.C84:015204,2011, 2011
This paper explores properties of baryons and finite density baryonic matter in an artificial world in which Nc, the number of colors, is large and the quarks of all species are degenerate and much larger than {\Lambda}_QCD. It has long been known that in large Nc QCD, baryons composed entirely of heavy quarks are accurately described in the mean-field
arxiv   +1 more source

Das zirkumgalaktische Medium

open access: yesPhysik in unserer Zeit, Volume 56, Issue 1, Page 30-37, January 2025.
Galaxien wie die Milchstraße sind umhüllt von einem gigantischen Kokon aus diffusem Gas. Aktuelle Forschungsergebnisse belegen, dass dieses zirkumgalakische Medium eine entscheidende Rolle für die Entstehung und Entwicklung von Galaxien spielt. Zusammenfassung Als zirkumgalaktisches Medium bezeichnet man die gasförmigen Hüllen von Galaxien, die sich ...
Philipp Richter
wiley   +1 more source

BARYON STRUCTURE [PDF]

open access: yesTheoretical Nuclear Physics in Italy, 2003
20 pages, no figures, invited general report at the "IX Convegno su Problemi di Fisica Nucleare e Teorica", Cortona, Oct.
openaire   +2 more sources

The eta' in baryon chiral perturbation theory

open access: yes, 2000
We include in a systematic way the eta' in baryon chiral perturbation theory. The most general relativistic effective Lagrangian describing the interaction of the lowest lying baryon octet with the Goldstone boson octet and the eta' is presented up to ...
B. Borasoy   +11 more
core   +1 more source

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