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Littérature scientifique sur le sujet « Baryons »

Auteur : Grafiati

Publié le 4 juin 2021

Mis à jour le 25 juillet 2025

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Articles de revues sur le sujet "Baryons"

1

GARCIA-RECIO, C., L. L. SALCEDO, D. GAMERMANN, J. NIEVES, O. ROMANETS, and L. TOLOS. "CHARMING BARYONS." International Journal of Modern Physics: Conference Series 26 (January 2014): 1460124. http://dx.doi.org/10.1142/s2010194514601240.

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We study odd-parity baryonic resonances with one heavy and three light flavors, dynamically generated by meson-baryon interactions. Special attention is paid to Heavy Quark Spin Symmetry (HQSS), hence pseudoscalar and vector mesons and baryons with Jπ = 1/2+ and 3/2+ are considered as constituent hadrons. For the hidden-charm sector ([Formula: see text]), the meson-baryon Lagrangian with Heavy Flavor Symmetry is constructed by a minimal extension of the SU(3) Weinberg-Tomozawa (WT) Lagrangian to fulfill HQSS, such that not new parameters are needed. This interaction can be presented in differe

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LEDDIG, TORSTEN. "INVESTIGATION OF B-MESON DECAYS INTO BARYONS WITH THE BABAR DETECTOR." International Journal of Modern Physics A 26, no. 03n04 (2011): 545–48. http://dx.doi.org/10.1142/s0217751x11051986.

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We report on investigations of B-meson decays into baryons with the BABAR detector. The comparison of different decay channels reveals that higher multiplicities are preferred for these decays. Furthermore, an enhancement in the invariant baryon-antibaryon mass distribution can be observed in several baryonic decay modes. In addition, the study of baryon resonances seen in baryonic B-meson decays is presented.

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Kostyuk, Ivan, Robert Lilow, and Matthias Bartelmann. "Baryon-photon interactions in Resummed Kinetic Field Theory." Journal of Cosmology and Astroparticle Physics 2023, no. 09 (2023): 032. http://dx.doi.org/10.1088/1475-7516/2023/09/032.

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Abstract We explore how interactions between baryons and photons can be incorporated into Kinetic Field Theory (KFT), a description of cosmic structure formation based on classical Hamiltonian particle dynamics. In KFT, baryons are described as effective mesoscopic particles which represent fluid elements governed by the hydrodynamic equations. In this paper, we modify the mesoscopic particle model to include pressure effects exerted on baryonic matter through interactions with photons. As a proof of concept, we use this extended mesoscopic model to describe the tightly coupled baryon-photon f

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Pardo Calderón, Leandro Manuel. "Baryon Acoustic Oscillations. Equation and physical interpretation." Scientia et Technica 23, no. 2 (2018): 263–68. http://dx.doi.org/10.22517/23447214.17251.

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Baryon Acoustic Oscillations are a phenomenon occurred before matter-radiation decoupling, characterized because the baryonic matter perturbation presents oscillations, as the name suggests. These perturbations propagate like a pressure wave on the photon-baryon ﬂuid produced by gravitational potentials, which join the baryonic matter, and collisions of baryons and photons, which scatter it. This paper shows the Baryon Acoustic Oscillations equation and it provides its physical meaning. Besides, it presents software CAMB as a tool to ﬁnd BAO equation solutions and support for its physical desc

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5

Dominguez-Tenreiro, Rosa, and Gustavo Yepes. "On the Possibility of a Higher Baryonic Contribution to Dark Matter." Symposium - International Astronomical Union 130 (1988): 592. http://dx.doi.org/10.1017/s0074180900137180.

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The most stringent constraint against baryonic dark matter is provided by primordial nucleosynthesis. Agreement between theory and observations is reachedonly for a limited range of the baryon-to-photon ratio ‘LR, namely , which implies that, in standard cosmological frameworks, the universe cannot be closed by baryons.

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Ghalenovi, Zahra. "Study of Heavy Strange Baryons in a Hypercentral Quark Model." International Journal of Modern Physics: Conference Series 46 (January 2018): 1860037. http://dx.doi.org/10.1142/s2010194518600376.

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In this work, we study the properties of the heavy baryons with strangeness employing a constituent quark model in the hypercentral approach. The potential model considers the interactions arising the one-gluon exchange, Goldstone boson exchange and confinement, aspects of underlying theory, quantum chromodynamics (QCD). By solving three-body Schrodinger equation of baryonic system, we obtain the ground as well as the corresponding energy eigenvalues of the system. Using the obtained energies, we calculate the baryon spectrum. We extend our scheme to predict the radiative decay width of the ch

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Wright, Ruby J., Claudia del P. Lagos, Chris Power, and Peter D. Mitchell. "The impact of stellar and AGN feedback on halo-scale baryonic and dark matter accretion in the eagle simulations." Monthly Notices of the Royal Astronomical Society 498, no. 2 (2020): 1668–92. http://dx.doi.org/10.1093/mnras/staa2359.

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ABSTRACT We use the eagle suite of hydrodynamical simulations to analyse accretion rates (and the breakdown of their constituent channels) on to haloes over cosmic time, comparing the behaviour of baryons and dark matter (DM). We also investigate the influence of sub-grid baryon physics on halo-scale inflow, specifically the consequences of modelling radiative cooling, as well as feedback from stars and active galactic nuclei (AGNs). We find that variations in halo baryon fractions at fixed mass (particularly their circumgalactic medium gas content) are very well correlated with variations in

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Khan, Mehbub, Yun Hao, and Jong-Ping Hsu. "Baryonic Force for Accelerated Cosmic Expansion and Generalized U1b Gauge Symmetry in Particle-Cosmology." EPJ Web of Conferences 168 (2018): 04004. http://dx.doi.org/10.1051/epjconf/201816804004.

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Based on baryon charge conservation and a generalized Yang-Mills symmetry for Abelian (and non-Abelian) groups, we discuss a new baryonic gauge field and its linear potential for two point-like baryon charges. The force between two point-like baryons is repulsive, extremely weak and independent of distance. However, for two extended baryonic systems, we have a dominant linear force α r. Thus, only in the later stage of the cosmic evolution, when two baryonic galaxies are separated by an extremely large distance, the new repulsive baryonic force can overcome the gravitational attractive force.

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HOSAKA, A., H. TOKI, and M. TAKAYAMA. "BARYON SPECTRA IN DEFORMED OSCILLATOR QUARK MODEL." Modern Physics Letters A 13, no. 21 (1998): 1699–707. http://dx.doi.org/10.1142/s0217732398001777.

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We study theoretically the baryon spectra in terms of a deformed oscillator quark (DOQ) model. This model is motivated by confinement of quarks and chiral symmetry breaking, which are the most important nonperturbative phenomena of QCD. The minimization of the DOQ Hamiltonian with respect to the deformation for each principal quantum number results in deformations for the intrinsic states of excited baryonic states. We find that the resulting baryon spectra agree very well with the existing experimental data including SU(3) baryons. The spatial deformation of the baryonic excited states carry

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McGaugh, Stacy S. "The Halo by Halo Missing Baryon Problem." Proceedings of the International Astronomical Union 3, S244 (2007): 136–45. http://dx.doi.org/10.1017/s1743921307013920.

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AbstractThe global missing baryon problem – that the sum of observed baryons falls short of the number expected form BBN – is well known. In addition to this, there is also a local missing baryon problem that applies to individual dark matter halos. This halo by halo missing baryon problem is such that the observed mass fraction of baryons in individual galaxies falls short of the cosmic baryon fraction. This deficit is a strong function of circular velocity. I give an empirical estimate of this function, and note the presence of a critical scale of ~ 900 km s−1 therein. I also briefly review

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Thèses sur le sujet "Baryons"

1

Urlichs, Konrad. "Baryons and baryonic matter in four-fermion interaction models." [S.l.] : [s.n.], 2007. http://deposit.ddb.de/cgi-bin/dokserv?idn=983572755.

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Ouared, Mohamed Rafik. "Étude des propriétés de production et de désintégration du baryon charme lambda C dans les interactions PP à 400 GeV/c." Paris 11, 1987. http://www.theses.fr/1987PA112191.

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Haupt, Christian. "Electromagnetic properties of baryons." [S.l.] : [s.n.], 2006. http://deposit.ddb.de/cgi-bin/dokserv?idn=980373271.

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Drach, Vincent. "Fermions twistés dynamiques et spectroscopie des baryons." Phd thesis, Grenoble, 2010. http://www.theses.fr/2010GRENY015.

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Ce travail s'intéresse au calcul de la masse des baryons à partir de la théorie décrivant l'interaction forte : la chromodynamique quantique (QCD). Cette théorie régit l'interaction entre les quarks et l es gluons et a pu durant ces dernières décennies être vérifiée à haute énergie grâce à l'une de ses propriétés : la liberté asymptoti que. Celle-ci prédit que les calculs perturbatifs sont valides à haute énergie car la constante de couplage tend vers zéro. Les quantités physiques régissant la physique à basse énergie nécessitent quant à elles un traitement non pertubatif et font l'objet de ce

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Drach, Vincent. "Fermions twistés dynamiques et spectroscopie des baryons." Phd thesis, Université de Grenoble, 2010. http://tel.archives-ouvertes.fr/tel-00633497.

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Ce travail s'intéresse au calcul de la masse des baryons à partir de la théorie décrivant l'interaction forte : la chromodynamique quantique (QCD). Cette théorie régit l'interaction entre les quarks et l es gluons et a pu durant ces dernières décennies être vérifiée à haute énergie grâce à l'une de ses propriétés : la liberté asymptoti que. Celle-ci prédit que les calculs perturbatifs sont valides à haute énergie car la constante de couplage tend vers zéro. Les quantités physiques régissant la physique à basse énergie nécessitent quant à elles un traitement non pertubatif et font l'objet de ce

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Habibi, Farhang. "Searching for missing baryons through scintillation." Phd thesis, Université Paris Sud - Paris XI, 2011. http://tel.archives-ouvertes.fr/tel-00625486.

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Cool molecular hydrogen H2 may be the ultimate possible constituent to the Milky-Way missing baryon. We describe a new way to search for such transparent matter in the Galactic disc and halo, through the diffractive and refractive effects on the light of background stars. By simulating the phase delay induced by a turbulent medium, we computed the corresponding illumination pattern on the earth for an extended source and a given passband. We show that in favorable cases, the light of a background star can be subjected to stochastic fluctuations of the order of a few percent at a characteristic

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Avenarius, Christoph. "The spin structure of the baryons." Thesis, University of Oxford, 1992. http://ora.ox.ac.uk/objects/uuid:448e060b-085d-449f-b33a-dd3913093d6d.

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Baryons are considered in the Nonrelativistic Quark Model (NQM) to be bound states of three valence quarks. Each quark has two possible spin eigenstates in the restframe of the baryon whose spin is fully carried by quarks. The baryon wavefunctions are connected through SU(6) symmetry rotations. For a long time, the measured magnetic moments of the baryons appeared to be in agreement with the NQM predictions. However, recent experiments which are examining the spin structure of the baryons show the failure of several NQM predictions. The so-called 'spin crisis' arose from the interpretation of

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MERLI, ANDREA. "SEARCH FOR CP VIOLATION IN BARYONS." Doctoral thesis, Università degli Studi di Milano, 2019. http://hdl.handle.net/2434/656029.

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In the past, flavour physics has driven indirect discoveries of new particles through precision measurements of other processes before the actual particles could be produced directly. For example the discovery of the differences in the behaviour of matter and antimatter, CP violation (CPV), has led to the explanation of flavour mixing with three families of quarks; the absence of the decay{KL}{mumu} decay drove the prediction of the cquark quark trough the GIM mechanism; the measurement of the Bd mixing allowed for the prediction of high mass of the quark quark. The asymmetry between matter

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Niemiec, Anna. "Influence of the environment on galaxy formation." Thesis, Aix-Marseille, 2017. http://www.theses.fr/2017AIXM0260/document.

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Dans le modèle de formation hiérarchique des structures, les amas de galaxies se forment et grandissent par l'accrétion de groupes plus petits ou de galaxies isolées. Dans ce scenario, comprendre comment les galaxies accrétées interagissent avec cet environnement très dense est une étape importante pour comprendre le schéma global de l'évolution des galaxies et de la formation des structures. En effet, pendant leur chute au coeur de l'amas, les galaxies sont sujettes à diverses interactions avec l'amas hôte, au niveau de leur composante baryonique aussi bien que matière noire, et ces interacti

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Knippschild, Bastian [Verfasser]. "Baryons in the chiral regime / Bastian Knippschild." Mainz : Universitätsbibliothek Mainz, 2012. http://d-nb.info/1020765712/34.

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Livres sur le sujet "Baryons"

1

Moshe, Gai, ed. Baryons '92. World Scientific, 1993.

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2

Barnes, Ted, and Hans-Peter Morsch. Baryon excitations: Lectures of the COSY workshop held at the Forschungszentrum Jülich from 2 to 3 May 2000. Forschungszentrum Jülich, Central Library, 2000.

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3

Weigel, H. Chiral soliton models for baryons. Springer, 2008.

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4

H, Toki, ed. Quarks, baryons and chiral symmetry. World Scientific, 2001.

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5

Mollerach, Silvia. Axino-induced baryogenesis. Fermi National Accelerator Laboratory, 1991.

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6

Esteban, Roulet, and United States. National Aeronautics and Space Administration., eds. Axino-induced baryogenesis. Fermi National Accelerator Laboratory, 1991.

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7

W, Wilson John. BRYNTRN: A baryon transport model. Langley Research Center, 1989.

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Mollerach, Silvia. Axino-induced baryogenesis. Fermi National Accelerator Laboratory, 1991.

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9

International Conference on the Structure of Baryons (12th 2010 Osaka, Japan). International Conference on the Structure of Baryons: (Baryons '10) : Osaka, Japan, 7-11 December 2010. Edited by Hosaka Atsushi. American Institute of Physics, 2011.

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10

Judd, Eleanor Gillian. Production of singly and doubly strange baryons and anti-baryons in heavy ion collisions at ultra-relativisticenergies. University of Birmingham, 1992.

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Chapitres de livres sur le sujet "Baryons"

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Povh, Bogdan, Klaus Rith, Christoph Scholz, Frank Zetsche, and Werner Rodejohann. "Baryons." In Graduate Texts in Physics. Springer Berlin Heidelberg, 2015. http://dx.doi.org/10.1007/978-3-662-46321-5_16.

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Amsler, Claude. "Baryons." In The Quark Structure of Hadrons. Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-98527-5_13.

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Carlson, C. E. "Perturbative QCD, Baryons, and Baryon Resonances." In New Aspects of Nuclear Dynamics. Springer US, 1989. http://dx.doi.org/10.1007/978-1-4613-0547-7_3.

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Povh, Bogdan, Klaus Rith, Christoph Scholz, and Frank Zetsche. "The Baryons." In Particles and Nuclei. Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-662-05432-1_15.

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Povh, Bogdan, Klaus Rith, Christoph Scholz, and Frank Zetsche. "The Baryons." In Particles and Nuclei. Springer Berlin Heidelberg, 1999. http://dx.doi.org/10.1007/978-3-642-87776-6_15.

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Povh, Bogdan, Klaus Rith, Christoph Scholz, and Frank Zetsche. "The Baryons." In Particles and Nuclei. Springer Berlin Heidelberg, 1995. http://dx.doi.org/10.1007/978-3-642-97653-7_15.

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Amsler, Claude. "Heavy Baryons." In The Quark Structure of Hadrons. Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-98527-5_17.

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Povh, Bogdan, Klaus Rith, Christoph Scholz, and Frank Zetsche. "The Baryons." In Particles and Nuclei. Springer Berlin Heidelberg, 2002. http://dx.doi.org/10.1007/978-3-662-05023-1_15.

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Capstick, Simon. "Missing Baryons." In N* Physics and Nonperturbative Quantum Chromodynamics. Springer Vienna, 1999. http://dx.doi.org/10.1007/978-3-7091-6800-4_15.

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de Freitas Pacheco, J. A. "Physics of Baryons." In The Cosmic Microwave Background. Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-44769-8_6.

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Actes de conférences sur le sujet "Baryons"

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Takeuchi, Sachiko, Makoto Takizawa, Kiyotaka Shimizu та ін. "Negative-parity Λ[sub Q] baryons in the baryon-meson continuum". У INTERNATIONAL CONFERENCE ON THE STRUCTURE OF BARYONS (BARYONS' 10). AIP, 2011. http://dx.doi.org/10.1063/1.3647409.

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MANOHAR, A. V. "BARYONS." In Phenomenology of Large NC QCD. WORLD SCIENTIFIC, 2002. http://dx.doi.org/10.1142/9789812776914_0015.

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MANOHAR, A. V. "BARYONS." In Proceedings of the Workshop. WORLD SCIENTIFIC, 2005. http://dx.doi.org/10.1142/9789812701725_0013.

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NAWA, KANABU, HIDEO SUGANUMA, ATSUSHI HOSAKA, and TORU KOJO. "BARYONS AND BARYONIC MATTER IN HOLOGRAPHIC QCD." In Hadron and Nuclear Physics 09. WORLD SCIENTIFIC, 2010. http://dx.doi.org/10.1142/9789814313933_0015.

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PAGE, P. R. "HYBRID BARYONS." In Proceedings of the 9th International Conference on the Structure of Baryons. WORLD SCIENTIFIC, 2003. http://dx.doi.org/10.1142/9789812704887_0021.

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Menze, D. W., and B. Metsch. "Baryons '98." In 8th International Conference. WORLD SCIENTIFIC, 1999. http://dx.doi.org/10.1142/9789814527491.

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Gibson, B. F., P. D. Barnes, J. B. McClelland, and W. Weise. "Baryons ’95." In 7th International Conference on the Structure of Baryons. WORLD SCIENTIFIC, 1996. http://dx.doi.org/10.1142/9789814531030.

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Gai, Moshe. "Baryons '92." In International Conference on the Structure of Baryons and Related Mesons. WORLD SCIENTIFIC, 1993. http://dx.doi.org/10.1142/9789814536950.

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LEBED, RICHARD F. "BARYONS, INC." In Proceedings of the Conference. WORLD SCIENTIFIC, 2004. http://dx.doi.org/10.1142/9789812702326_0005.

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Yi, Piljin, Atsushi Hosaka, Kanchan Khemchandani, Hideko Nagahiro, and Kanabu Nawa. "Precision Holographic Baryons." In INTERNATIONAL CONFERENCE ON THE STRUCTURE OF BARYONS (BARYONS' 10). AIP, 2011. http://dx.doi.org/10.1063/1.3647358.

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Rapports d'organisations sur le sujet "Baryons"

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Mukhopadhyay, N. C. Excited baryons. Office of Scientific and Technical Information (OSTI), 1986. http://dx.doi.org/10.2172/6901547.

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Gibney, Mark C. Photoproduction of Charmed Baryons. Office of Scientific and Technical Information (OSTI), 1989. http://dx.doi.org/10.2172/1427791.

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Gibney, Mark C. Photoproduction of Charmed Baryons. Office of Scientific and Technical Information (OSTI), 1989. http://dx.doi.org/10.2172/1156311.

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Swiatek, Joseph Alexander. A Study of charm baryons containing a lambda baryon in the final state. Office of Scientific and Technical Information (OSTI), 1995. http://dx.doi.org/10.2172/1423680.

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Bjorken, James. Masses of charm and strange baryons. Office of Scientific and Technical Information (OSTI), 1986. http://dx.doi.org/10.2172/1163145.

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Mattson, Mark Edward. Search for Baryons with Two Charm Quarks. Office of Scientific and Technical Information (OSTI), 2002. http://dx.doi.org/10.2172/1420963.

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Summers, D. J. Charm strange baryons and the 1.5 prong. Office of Scientific and Technical Information (OSTI), 1992. http://dx.doi.org/10.2172/10125015.

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Lanza, Lucille. Search for hybrid baryons with CLAS12 experimental setup. Office of Scientific and Technical Information (OSTI), 2017. http://dx.doi.org/10.2172/1369432.

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Vaandering, Eric Wayne. Mass and Width Measurements of $\Sigma_{c}$ Baryons. Office of Scientific and Technical Information (OSTI), 2000. http://dx.doi.org/10.2172/1421442.

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Torres Aguilar, Ibrahim Daniel. Observation of Double Charm Baryons in Several decay Modes. Office of Scientific and Technical Information (OSTI), 2006. http://dx.doi.org/10.2172/1415801.

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