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Relevant bibliographies by topics / Scalar relativistic

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Academic literature on the topic 'Scalar relativistic'

Author: Grafiati

Published: 4 June 2021

Last updated: 7 February 2022

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Journal articles on the topic "Scalar relativistic"

1

Davis, Simon. "Relativistic Quantum Scalar Fields." Bulletin of Pure & Applied Sciences- Physics 40d, no. 1 (2021): 25–33. http://dx.doi.org/10.5958/2320-3218.2021.00003.8.

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Gomes, M., J. M. C. Malbouisson, A. G. Rodrigues, and A. J. da Silva. "Relativistic scalar Aharonov-Bohm scattering." Journal of Physics A: Mathematical and General 33, no. 31 (2000): 5521–29. http://dx.doi.org/10.1088/0305-4470/33/31/307.

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Mitchell, D. B., Y. Nogami, and N. D. Whelan. "Relativistic versus nonrelativistic Hartree–Fock calculations: solvable examples in one dimension." Canadian Journal of Physics 67, no. 6 (1989): 583–86. http://dx.doi.org/10.1139/p89-106.

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Relativistic and nonrelativistic one-dimensional systems of particles of the same mass interacting through instantaneous contact interactions are considered. For the relativistic interaction, we assume a combination of a Lorentz scalar and a vector. The mass and interaction strength are chosen such that the deuteron is simulated; the relativistic and nonrelativistic "deuteron" models have the same binding energy and practically the same structure. The relativistic and nonrelativistic Hartree–Fock equations can both be solved analytically. For certain combinations of the Lorentz scalar and vect

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Bischoff, Florian A., Edward F. Valeev, Wim Klopper, and Curtis L. Janssen. "Scalar relativistic explicitly correlated R12 methods." Journal of Chemical Physics 132, no. 21 (2010): 214104. http://dx.doi.org/10.1063/1.3417984.

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Kamiński, R., L. Leśniak, and J. P. Maillet. "Relativistic effects in scalar meson dynamics." Physical Review D 50, no. 5 (1994): 3145–57. http://dx.doi.org/10.1103/physrevd.50.3145.

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Hussain, T., M. Khurshudyan, S. Ahmed, and As Khurshudyan. "Role of structure scalars on viscous and heat conducting spherical systems in f(R,T) gravity." International Journal of Modern Physics D 26, no. 14 (2017): 1750155. http://dx.doi.org/10.1142/s0218271817501553.

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In this paper, we analyze some dynamical features of spherical celestial objects through structure scalars in [Formula: see text] gravitational theory, where [Formula: see text] and [Formula: see text] are the Ricci scalar and the trace of energy–momentum tensor, respectively. In this framework, we consider our relativistic geometry to be spherical in shape filled with radiating viscous and shearing fluid content. We formulate extended version of structure scalars by orthogonal decomposition of the Riemann tensor with and without constant [Formula: see text] and [Formula: see text] backgrounds

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ROŻYNEK, JACEK. "THE NUCLEAR SCALAR POTENTIAL AND THE EMC EFFECT." International Journal of Modern Physics E 09, no. 03 (2000): 195–203. http://dx.doi.org/10.1142/s0218301300000155.

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Based on the relativistic mean field model of nuclear matter with scalar and vector components, a convolution model of deeply inelastic electron-nucleus scattering has been developed. The influence of the scalar potential changes the nucleon structure function inside the nucleus and ensures agreement with the experiment in the Björken x>0.2. The Sum Rules are discussed. The role of the relativistic scalar and vector nuclear potential in the nucleus is shown.

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Jarvis, P. D., and I. Tsohantjis. "Covariant scalar representation of and quantization of the scalar relativistic particle." Journal of Physics A: Mathematical and General 29, no. 6 (1996): 1245–60. http://dx.doi.org/10.1088/0305-4470/29/6/011.

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BERTOLAMI, ORFEU. "DARK ENERGY, DARK MATTER AND GRAVITY." International Journal of Modern Physics D 16, no. 12a (2007): 2003–12. http://dx.doi.org/10.1142/s0218271807011218.

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We discuss the motivation for high accuracy relativistic gravitational experiments in the solar system and complementary cosmological tests. We focus our attention on the issue of distinguishing a generic scalar theory of gravity as the underlying physical theory from the usual general-relativistic picture, where one expects the presence of fundamental scalar fields associated, for instance, with inflation, dark matter and dark energy.

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Ahmad, S., A. Rehman Jami, and Z. Aas. "Shear and expansion evolution for dissipative fluids." Modern Physics Letters A 33, no. 20 (2018): 1850111. http://dx.doi.org/10.1142/s0217732318501110.

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The aim of this work is to analyze the role of shear evolution equation in the modeling of relativistic spheres in f(R) gravity. We assume that non-static diagonally symmetric geometry is coupled with dissipative anisotropic viscous fluid distributions in the presence of f(R) dark source terms. A specific distribution of f(R) cosmic model has been assumed and the spherical mass function through generic formula introduced by Misner–Sharp has been formulated. Some very important relations regarding Weyl scalar, matter variables and mass functions are being computed. After decomposing orthogonall

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Dissertations / Theses on the topic "Scalar relativistic"

1

Krtous, Pavel. "Relationships between scalar field and relativistic particle quantizations." Thesis, National Library of Canada = Bibliothèque nationale du Canada, 1997. http://www.collectionscanada.ca/obj/s4/f2/dsk3/ftp04/nq23010.pdf.

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Nedjadi, Youcef. "Elektroweak tests of the relativistic nuclear scalar-vector model." Thesis, University of Oxford, 1989. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.236201.

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Vrettea, Christine. "Relativistic scattering theory with a vector potential." Thesis, Keele University, 2002. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.268335.

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Khandogin, Yang. "Nonrelativistic and scalar relativistic nuclear spin-spin couplings in density functional theory." Thesis, National Library of Canada = Bibliothèque nationale du Canada, 1999. http://www.collectionscanada.ca/obj/s4/f2/dsk1/tape7/PQDD_0017/MQ48017.pdf.

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Díaz, Calzadilla Pablo. "Scalar stars and effective field theory." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2021. http://amslaurea.unibo.it/23167/.

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The axion is one of the favored candidates to form the cold dark matter in the universe. This pseudo-scalar field may form compact objects called axion stars, whose physics is well captured by means of non-relativistic effective field theory coupled to Newtonian gravity. The interplay between gradient energy, self-interactions and gravity gives rise to both dilute and dense axion stars. While the existence of the dilute axion stars is well established, the situation is more complicated in the case of the so-called dense axion stars, an extra physically stable solution of the system of differen

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Stokley, Martin. "An investigation into particle and field ontologies for relativistic scalar fields in de Broglie-Bohm type theories." Thesis, University of Portsmouth, 2001. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.343394.

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Feix, Martin. "Extragalactic and cosmological tests of gravity theories with additional scalar or vector fields." Thesis, University of St Andrews, 2011. http://hdl.handle.net/10023/1901.

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Despite the many successes of the current standard model of cosmology on the largest physical scales, it relies on two phenomenologically motivated constituents, cold dark matter and dark energy, which account for approximately 95% of the energy-matter content of the universe. From a more fundamental point of view, however, the introduction of a dark energy (DE) component is theoretically challenging and extremely fine-tuned, despite the many proposals for its dynamics. On the other hand, the concept of cold dark matter (CDM) also suffers from several issues such as the lack of direct experime

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Rinskopf, Nathalie. "Etude ab initio des effets de corrélation et des effets relativistes dans les halogénures diatomiques de métaux de transition." Doctoral thesis, Universite Libre de Bruxelles, 2007. http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/210678.

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Ce travail est une contribution ab initio à la caractérisation d'halogénures diatomiques de métaux de transition. Nous avons choisi de caractériser la structure électronique des chlorures de métaux de transition du groupe Vb (NbCl et TaCl) et du fluorure de nickel car une série de spectres les concernant ont été enregistrés mais aucune donnée théorique fiable n'était disponible dans la littérature.<p><p>Pour étudier ces molécules, nous avons appliqué une procédure de calcul à deux étapes qui permet de tenir compte des effets de corrélation électronique et des effets relativistes. Dans la premi

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Duniya, Didam Gwazah Adams. "Relativistic corrections to the power spectrum." University of the Western Cape, 2015. http://hdl.handle.net/11394/4787.

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Philosophiae Doctor - PhD<br>The matter power spectrum is key to understanding the growth of large-scale structure in the Universe. Upcoming surveys of galaxies in the optical and HI will probe increasingly large scales, approaching and even exceeding the Hubble scale at the survey redshifts. On these cosmological scales, surveys can in principle provide the best constraints on dark energy (DE) and modified gravity models and will be able to test general relativity itself. However, in order to realise the potential of these surveys, we need to ensure that we are using a correct analysis, i.e.

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Mourier, Pierre. "Cosmologie inhomogène relativiste : modèles non perturbatifs et moyennes spatiales des équations d’Einstein." Thesis, Lyon, 2019. http://www.theses.fr/2019LYSE1116/document.

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Dans le modèle standard de la cosmologie, la dynamique globale de l'Univers est modélisée par l'intermédiaire d'un espace-temps de référence (ou de fond) fortement symétrique, admettant des sections spatiales homogènes et isotropes. Le couplage entre les sources fluides, homogènes, et l'expansion globale, y est déterminé par les équations d'Einstein de la Relativité Générale. La formation de structures inhomogènes de matière peut également être décrite dans ce modèle. Selon l'époque et l'échelle considérées, cette description est effectuée soit à l'aide d'un schéma perturbatif relativiste supp

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Books on the topic "Scalar relativistic"

1

Stokley, Martin. An investigation into particle and field ontologies for relativistic scalar fields in de Broglie-Bohm type theories. University of Portsmouth, 2001.

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2

Introduction to General Relativistic and Scalar-Tensor Cosmologies. Nova Science Publishers, 2007.

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3

Baulieu, Laurent, John Iliopoulos, and Roland Sénéor. Relativistic Wave Equations. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780198788393.003.0006.

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Relativistically covariant wave equations for scalar, spinor, and vector fields. Plane wave solutions and Green’s functions. The Klein–Gordon equation. The Dirac equation and the Clifford algebra of γ‎ matrices. Symmetries and conserved currents. Hamiltonian and Lagrangian formulations. Wave equations for spin-1 fields.

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Deruelle, Nathalie, and Jean-Philippe Uzan. The classical scalar field. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198786399.003.0027.

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This chapter explains some of the properties of scalar fields, which are paradigmatic in relativistic field theory. It also shows how a complex scalar field can confer an effective mass to a ‘gauge’ field. The chapter first provides the Klein–Gordon equation derived from the Euler–Lagrange equations outlined in the previous chapter. It then illustrates the Fourier transform of a free field, before embarking on further discussions on complex fields, charge, and symmetry breaking. Finally, this chapter considers that the fact that global symmetry breaking leads to the appearance of a massless, a

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5

Franz, Gross, Continuous Electron Beam Accelerator Facility., and United States. National Aeronautics and Space Administration., eds. Pseudo-scalar [symbol for pi] N coupling and relativistic proton-nucleus scattering. Continuous Electron Beam Accelerator Facility, 1989.

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Franz, Gross, Continuous Electron Beam Accelerator Facility., and United States. National Aeronautics and Space Administration., eds. Pseudo-scalar [symbol for pi] N coupling and relativistic proton-nucleus scattering. Continuous Electron Beam Accelerator Facility, 1989.

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Pseudo-scalar [symbol for pi] N coupling and relativistic proton-nucleus scattering. Continuous Electron Beam Accelerator Facility, 1989.

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Franz, Gross, Continuous Electron Beam Accelerator Facility., and United States. National Aeronautics and Space Administration., eds. Pseudo-scalar [symbol for pi] N coupling and relativistic proton-nucleus scattering. Continuous Electron Beam Accelerator Facility, 1989.

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9

Succi, Sauro. The Lattice Boltzmann Equation. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780199592357.001.0001.

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Over the past near three decades, the Lattice Boltzmann method has gained a prominent role as an efficient computational method for the numerical simulation of a wide variety of complex states of flowing matter across a broad range of scales, from fully developed turbulence, to multiphase micro-flows, all the way down to nano-biofluidics and lately, even quantum-relativistic subnuclear fluids. After providing a self-contained introduction to the kinetic theory of fluids and a thorough account of its transcription to the lattice framework, this book presents a survey of the major developments w

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Deruelle, Nathalie, and Jean-Philippe Uzan. Cosmological perturbations. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198786399.003.0061.

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This chapter describes the first steps toward an understanding of large structures, which are observed in the universe at all scales—galaxies, groups of galaxies, and galactic clusters. It does so by studying the evolution of perturbations at linear order in Friedmann–Lemaître spacetimes. To simplify the discussion, the chapter limits the scope to the textbook case where the spatial sections of the background space are Euclidean (K = 0), and anisotropic perturbations and entropy perturbations are absent. This basically means that the matter reduces to a single fluid. The relativistic and Newto

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Book chapters on the topic "Scalar relativistic"

1

Stone, Michael. "Relativistic Scalar Fields." In Graduate Texts in Contemporary Physics. Springer New York, 2000. http://dx.doi.org/10.1007/978-1-4612-0507-4_2.

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2

Woit, Peter. "Symmetries and Relativistic Scalar Quantum Fields." In Quantum Theory, Groups and Representations. Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-64612-1_44.

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Komar, Arthur. "Normal Mode Quantization of Relativistic Scalar Fields in an Einstein Elevator." In Advances in the Interplay Between Quantum and Gravity Physics. Springer Netherlands, 2002. http://dx.doi.org/10.1007/978-94-010-0347-6_10.

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Duviryak, A. "Heuristic Model of Two-Quark Relativistic System with Scalar-Vector Interaction." In Few-Body Problems in Physics ’02. Springer Vienna, 2003. http://dx.doi.org/10.1007/978-3-7091-6728-1_97.

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Cassing, Wolfgang, and Sascha Juchem. "Correlations and Equilibration in Relativistic Quantum Systems." In Nonequilibrium Physics at Short Time Scales. Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-662-08990-3_10.

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Moisson, X. "Links Between Time Scales Using Barycentric Relativistic Ephemerides." In The Dynamical Behaviour of our Planetary System. Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-011-5510-6_23.

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Dennett-Thorpe, J. "Relativistic Motion on Kilo-Parsec Scales in Powerful Radio Sources." In The Non-Sleeping Universe. Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4497-1_60.

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Sazhin, S. S., A. E. Sumner, and N. M. Temme. "Are relativistic effects significant for the analysis of whistler-mode waves in the earth's magnetosphere?" In Space Plasmas: Coupling Between Small and Medium Scale Processes. American Geophysical Union, 1995. http://dx.doi.org/10.1029/gm086p0139.

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Stock, Reinhard. "Relativistic Nucleus-Nucleus Collisions and the QCD Matter Phase Diagram." In Particle Physics Reference Library. Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-38207-0_7.

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AbstractThis review will be concerned with our knowledge of extended matter under the governance of strong interaction, in short: QCD matter. Strictly speaking, the hadrons are representing the first layer of extended QCD architecture. In fact we encounter the characteristic phenomena of confinement as distances grow to the scale of 1 fm (i.e. hadron size): loss of the chiral symmetry property of the elementary QCD Lagrangian via non-perturbative generation of “massive” quark and gluon condensates, that replace the bare QCD vacuum. However, given such first experiences of transition from short range perturbative QCD phenomena (jet physics etc.), toward extended, non perturbative QCD hadron structure, we shall proceed here to systems with dimensions far exceeding the force range: matter in the interior of heavy nuclei, or in neutron stars, and primordial matter in the cosmological era from electro-weak decoupling (10−12 s) to hadron formation (0.5 ⋅ 10−5 s). This primordial matter, prior to hadronization, should be deconfined in its QCD sector, forming a plasma (i.e. color conducting) state of quarks and gluons: the Quark Gluon Plasma (QGP).

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Zinn-Justin, Jean. "The neutral relativistic scalar field." In Quantum Field Theory and Critical Phenomena. Oxford University Press, 2021. http://dx.doi.org/10.1093/oso/9780198834625.003.0006.

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This chapter introduces the relativistic quantum field theory (QFT) of the neutral scalar boson field. It is a local, relativistic invariant, theory for a real field extension of the non-relativistic field theory of the Bose gas. Locality is a property that plays a central role in most of this work. The QFT is discussed both from the viewpoint of real-time evolution and statistical physics. The holomorphic formalism leads to representations of the S-matrix in terms of field integrals. The S-matrix elements are related to the continuation to real time of various kinds of Euclidean correlation functions. It is argued that the massive φ<sup>4</sup> QFT has the quantum Bose gas with a pair potential, in the grand canonical formulation, as a non-relativistic limit.

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Conference papers on the topic "Scalar relativistic"

1

Wang, Chih-Hung, Da-Shin Lee, Wolung Lee, and She-Sheng Xue. "Spinning Particles in Scalar-Tensor Gravity with Torsion." In RELATIVISTIC ASTROPHYSICS: 5th Sino-Italian Workshop on Relativistic Astrophysics. AIP, 2008. http://dx.doi.org/10.1063/1.3012269.

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Sahariya, Jagrati, and H. S. Mund. "Electronic structure of FeTiSb using relativistic and scalar-relativistic approaches." In INTERNATIONAL CONFERENCE ON CONDENSED MATTER AND APPLIED PHYSICS (ICC 2015): Proceeding of International Conference on Condensed Matter and Applied Physics. Author(s), 2016. http://dx.doi.org/10.1063/1.4946643.

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Gordon, Christopher. "Entropy and adiabatic components in scalar field perturbations." In RELATIVISTIC ASTROPHYSICS: 20th Texas Symposium. AIP, 2001. http://dx.doi.org/10.1063/1.1419536.

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Frolov, Andrei V. "Critical collapse of a massless scalar field: Perturbative approach." In GENERAL RELATIVITY AND RELATIVISTIC ASTROPHYSICS. ASCE, 1999. http://dx.doi.org/10.1063/1.1301576.

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TAKANO NATTI, E. R., P. L. NATTI, and C. Y. LIN. "BOUND STATES OF A RELATIVISTIC SCALAR PLASMA SYSTEM." In Proceedings of the VIII International Workshop. WORLD SCIENTIFIC, 2003. http://dx.doi.org/10.1142/9789812704429_0073.

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Noble, Adam, and Dino A. Jaroszynski. "Electrostatic and scalar fields." In Relativistic Plasma Waves and Particle Beams as Coherent and Incoherent Radiation Sources IV, edited by Dino A. Jaroszynski and MinSup Hur. SPIE, 2021. http://dx.doi.org/10.1117/12.2595296.

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Lecian, O. M., G. Montani, Carlo Luciano Bianco, and She-Sheng Xue. "Scalar-tensor analysis of an exponential Lagrangian for the Gravitational Field." In RELATIVISTIC ASTROPHYSICS: 4th Italian-Sino Workshop. AIP, 2008. http://dx.doi.org/10.1063/1.2837006.

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Lee, Hee-Jung. "A QCD sum rule study of two scalar mesons f0(980) and a0(980)." In Light Cone 2010: Relativistic Hadronic and Particle Physics. Sissa Medialab, 2010. http://dx.doi.org/10.22323/1.119.0067.

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KOSIŃSKI, PIOTR, PAWEŁ MAŚLANKA, JERZY LUKIERSKI та ANDRZEJ SITARZ. "GENERALIZED κ-DEFORMATIONS AND DEFORMED RELATIVISTIC SCALAR FIELDS ON NONCOMMUTATIVE MINKOWSKI SPACE". У Proceedings of 2002 International Conference. WORLD SCIENTIFIC, 2006. http://dx.doi.org/10.1142/9789812772732_0022.

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Marcos, S., M. López-Quelle, R. Niembro, and L. N. Savushkin. "Nuclear relativistic Hartree-Fock calculations including pions interacting with a scalar field." In NUCLEAR STRUCTURE AND DYNAMICS 2012. AIP, 2012. http://dx.doi.org/10.1063/1.4764251.

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Reports on the topic "Scalar relativistic"

1

Lyutikov, M. Polarization and Structure of Relativistic Parsec-Scale AGN Jets. Office of Scientific and Technical Information (OSTI), 2004. http://dx.doi.org/10.2172/826966.

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