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Journal articles on the topic 'Matter models'

To see the other types of publications on this topic, follow the link: Matter models.

Author: Grafiati

Published: 14 March 2023

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1

Sozmen, Elif G., Jason D. Hinman, and S. Thomas Carmichael. "Models That Matter: White Matter Stroke Models." Neurotherapeutics 9, no. 2 (February 24, 2012): 349–58. http://dx.doi.org/10.1007/s13311-012-0106-0.

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2

Takibayev, N. "Models of dark particle interactions with ordinary matter." Physical Sciences and Technology 2, no. 2 (2015): 58–69. http://dx.doi.org/10.26577/2409-6121-2015-2-2-58-69.

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3

Kristensen, Kai, Hans J. Juhl, and Jacob Eskildsen. "Models that matter." International Journal of Business Performance Management 5, no. 1 (2003): 91. http://dx.doi.org/10.1504/ijbpm.2003.002102.

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4

Morgante, Enrico. "Simplified Dark Matter Models." Advances in High Energy Physics 2018 (December 17, 2018): 1–13. http://dx.doi.org/10.1155/2018/5012043.

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I review the construction of simplified models for dark matter searches. After discussing the philosophy and some simple examples, I turn the attention to the aspect of the theoretical consistency and to the implications of the necessary extensions of these models.

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5

Foot, R. "Generalized mirror matter models." Physics Letters B 632, no. 4 (January 2006): 467–70. http://dx.doi.org/10.1016/j.physletb.2005.10.074.

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6

Atiyah, M. F., N. S. Manton, and B. J. Schroers. "Geometric models of matter." Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences 468, no. 2141 (January 5, 2012): 1252–79. http://dx.doi.org/10.1098/rspa.2011.0616.

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Inspired by soliton models, we propose a description of static particles in terms of Riemannian 4-manifolds with self-dual Weyl tensor. For electrically charged particles, the 4-manifolds are non-compact and asymptotically fibred by circles over physical 3-space. This is akin to the Kaluza–Klein description of electromagnetism, except that we exchange the roles of magnetic and electric fields, and only assume the bundle structure asymptotically, away from the core of the particle in question. We identify the Chern class of the circle bundle at infinity with minus the electric charge and, at least provisionally, the signature of the 4-manifold with the baryon number. Electrically neutral particles are described by compact 4-manifolds. We illustrate our approach by studying the Taub–Newman, Unti, Tamburino (Taub–NUT) manifold as a model for the electron, the Atiyah–Hitchin manifold as a model for the proton, with the Fubini–Study metric as a model for the neutron and S 4 with its standard metric as a model for the neutrino.

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7

Neff, Ellen P. "Models matter in metastasis." Lab Animal 46, no. 1 (January 2017): 3. http://dx.doi.org/10.1038/laban.1170.

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8

Anker, Suzanne, Kevin Clarke, Agnes Denes, Michael Joaquín Grey, Ruth Kavenoff, Thomas Kovachemch, David Kremers, et al. "Models, Metaphors, and Matter." Art Journal 55, no. 1 (March 1996): 33–43. http://dx.doi.org/10.1080/00043249.1996.10791737.

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9

Phillips, Kimberley A., Karen L. Bales, John P. Capitanio, Alan Conley, Paul W. Czoty, Bert A. ‘t Hart, William D. Hopkins, et al. "Why primate models matter." American Journal of Primatology 76, no. 9 (April 10, 2014): 801–27. http://dx.doi.org/10.1002/ajp.22281.

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10

Blinnikov, Sergei I. "Mirror matter and other dark matter models." Uspekhi Fizicheskih Nauk 184, no. 2 (2014): 194–99. http://dx.doi.org/10.3367/ufnr.0184.201402h.0194.

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11

Blinnikov, S. I. "Mirror matter and other dark matter models." Physics-Uspekhi 57, no. 2 (February 28, 2014): 183–88. http://dx.doi.org/10.3367/ufne.0184.201402h.0194.

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12

Bormotova, I. M., and E. M. Kopteva. "Friedmann Cosmological Models with Various Equations of State of Matter." Ukrainian Journal of Physics 61, no. 9 (September 2016): 843–49. http://dx.doi.org/10.15407/ujpe61.09.0843.

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13

Arnowitt, R., B. Dutta, and Y. Santoso. "Dark matter in Susy models." Physics of Atomic Nuclei 65, no. 12 (December 2002): 2218–24. http://dx.doi.org/10.1134/1.1530303.

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14

Thirukkanesh, S., and S. D. Maharaj. "Exact models for isotropic matter." Classical and Quantum Gravity 23, no. 7 (March 17, 2006): 2697–709. http://dx.doi.org/10.1088/0264-9381/23/7/028.

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15

Maddox, John. "Refining models of nuclear matter." Nature 362, no. 6419 (April 1993): 407. http://dx.doi.org/10.1038/362407a0.

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16

Maguire, John F. "Process Models for Interfacial Matter." IFAC Proceedings Volumes 31, no. 29 (October 1998): 119–26. http://dx.doi.org/10.1016/s1474-6670(17)38932-2.

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17

Hadeler, K. P., and Christina Kuttler. "Dynamical models for granular matter." Granular Matter 2, no. 1 (August 1999): 9–18. http://dx.doi.org/10.1007/s100350050029.

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18

Arnowitt, R., and Pran Nath. "Models of particle dark matter." Nuclear Physics B - Proceedings Supplements 51, no. 2 (November 1996): 171–77. http://dx.doi.org/10.1016/s0920-5632(96)00501-4.

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19

Shaebani, M. Reza, Adam Wysocki, Roland G. Winkler, Gerhard Gompper, and Heiko Rieger. "Computational models for active matter." Nature Reviews Physics 2, no. 4 (March 10, 2020): 181–99. http://dx.doi.org/10.1038/s42254-020-0152-1.

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20

Shanenko, A. A., E. P. Yukalova, and V. I. Yukalov. "Statistical models of clustering matter." Physica A: Statistical Mechanics and its Applications 197, no. 4 (August 1993): 629–66. http://dx.doi.org/10.1016/0378-4371(93)90020-5.

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21

Horowitz, C. J., and J. Piekarewicz. "Quark models of nuclear matter." Nuclear Physics A 536, no. 3-4 (January 1992): 669–96. http://dx.doi.org/10.1016/0375-9474(92)90118-4.

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22

Bertacca, Daniele, Nicola Bartolo, and Sabino Matarrese. "Unified Dark Matter Scalar Field Models." Advances in Astronomy 2010 (2010): 1–29. http://dx.doi.org/10.1155/2010/904379.

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We analyze and review cosmological models in which the dynamics of a single scalar field accounts for a unified description of the Dark Matter and Dark Energy sectors, dubbed Unified Dark Matter (UDM) models. In this framework, we consider the general Lagrangian of -essence, which allows to find solutions around which the scalar field describes the desired mixture of Dark Matter and Dark Energy. We also discuss static and spherically symmetric solutions of Einstein's equations for a scalar field with noncanonical kinetic term, in connection with galactic halo rotation curves.

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23

Hollander, Elizabeth. "Subject Matter: Models for Different Media." Representations 36, no. 1 (October 1991): 133–46. http://dx.doi.org/10.1525/rep.1991.36.1.99p00867.

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24

Hollander, Elizabeth. "Subject Matter: Models for Different Media." Representations 36 (1991): 133–46. http://dx.doi.org/10.2307/2928635.

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25

Liddle, A. R., and D. H. Lyth. "Inflation and mixed dark matter models." Monthly Notices of the Royal Astronomical Society 265, no. 2 (November 15, 1993): 379–84. http://dx.doi.org/10.1093/mnras/265.2.379.

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26

Muñoz, Carlos. "Models of Supersymmetry for Dark Matter." EPJ Web of Conferences 136 (2017): 01002. http://dx.doi.org/10.1051/epjconf/201713601002.

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27

Campos, A., G. Yepes, A. Klypin, G. Murante, A. Provenzale, and S. Borgani. "Mass Segregation in Dark Matter Models." Astrophysical Journal 446 (June 1995): 54. http://dx.doi.org/10.1086/175766.

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28

Chiba, Takeshi, Naoshi Sugiyama, and Takashi Nakamura. "Observational tests of x-matter models." Monthly Notices of the Royal Astronomical Society 301, no. 1 (November 1998): 72–80. http://dx.doi.org/10.1046/j.1365-8711.1998.02012.x.

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29

Olive, Keith A. "Dark Matter in SuperGUT Unification Models." Journal of Physics: Conference Series 315 (August 19, 2011): 012021. http://dx.doi.org/10.1088/1742-6596/315/1/012021.

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30

Fukuma, Masafumi, Sotaro Sugishita, and Naoya Umeda. "Matter fields in triangle–hinge models." Progress of Theoretical and Experimental Physics 2016, no. 5 (May 2016): 053B04. http://dx.doi.org/10.1093/ptep/ptw051.

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31

Tod, K. P. "Isotropic cosmological singularities: other matter models." Classical and Quantum Gravity 20, no. 3 (January 15, 2003): 521–34. http://dx.doi.org/10.1088/0264-9381/20/3/309.

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32

Muñoz, Carlos. "Indirect dark matter searches and models." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 692 (November 2012): 13–19. http://dx.doi.org/10.1016/j.nima.2012.01.053.

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33

Rodolfa, Emil R., Nadine J. Kaslow, Alan E. Stewart, W. Gregory Keilin, and Jeff Baker. "Internship training: Do models really matter?" Professional Psychology: Research and Practice 36, no. 1 (February 2005): 25–31. http://dx.doi.org/10.1037/0735-7028.36.1.25.

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34

DUTRA, M., O. LOURENÇO, A. DELFINO, and J. S. SÁ MARTINS. "SKYRME MODELS AND NUCLEAR MATTER PROPERTIES." International Journal of Modern Physics D 19, no. 08n10 (August 2010): 1583–86. http://dx.doi.org/10.1142/s0218271810017937.

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In this preliminary study we select a set of six Skyrme models which present reasonable symmetry energies lying in the range of 28–35 MeV to analyze the behavior of several other bulk properties at zero temperature, as well as the critical temperature parameters. The models are also investigated to see whether they satisfy a stringent constraint recently proposed from heavy-ion experiments.

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35

Suematsu, Daijiro. "Neutrino mass models and dark matter." Progress in Particle and Nuclear Physics 64, no. 2 (April 2010): 454–56. http://dx.doi.org/10.1016/j.ppnp.2009.12.074.

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36

Vorms, Marion. "Representing with imaginary models: Formats matter." Studies in History and Philosophy of Science Part A 42, no. 2 (June 2011): 287–95. http://dx.doi.org/10.1016/j.shpsa.2010.11.036.

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37

Bergström, Lars. "Dark matter: Models and detection methods." Nuclear Physics B - Proceedings Supplements 118 (April 2003): 329–40. http://dx.doi.org/10.1016/s0920-5632(03)01326-4.

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38

LI, TianJun, ZhaoFeng KANG, and Xin GAO. "Introduction to the dark matter models." SCIENTIA SINICA Physica, Mechanica & Astronomica 41, no. 12 (November 1, 2011): 1396–401. http://dx.doi.org/10.1360/132011-976.

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39

Cheung, Clifford, and David Sanford. "Simplified models of mixed dark matter." Journal of Cosmology and Astroparticle Physics 2014, no. 02 (February 6, 2014): 011. http://dx.doi.org/10.1088/1475-7516/2014/02/011.

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40

van Holten, J. W. "Matter coupling in supersymmetric σ-models." Nuclear Physics B 260, no. 1 (October 1985): 125–35. http://dx.doi.org/10.1016/0550-3213(85)90314-1.

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41

MURANTE, G., A. PROVENZALE, S. BORGANI, A. CAMPOS, and G. YEPES. "Scaling analysis of dark matter models." Astroparticle Physics 5, no. 1 (June 1996): 53–68. http://dx.doi.org/10.1016/0927-6505(96)00005-9.

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42

Lee, T. H. "Making models matter — Lessons from experience." European Journal of Operational Research 38, no. 3 (February 1989): 290–300. http://dx.doi.org/10.1016/0377-2217(89)90006-4.

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43

ABDUSSATTAR. "COSMOLOGICAL MODELS GENERALIZING ROBERTSON–WALKER MODELS." International Journal of Modern Physics D 12, no. 09 (October 2003): 1603–13. http://dx.doi.org/10.1142/s021827180300433x.

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Considering the physical 3-space t= constant of the space–time metrics as spheroidal and pseudo-spheroidal, cosmological models which are generalizations of Robertson–Walker models are obtained. Specific forms of these general models as solutions of Einstein's field equations are also discussed in the radiation and the matter dominated era of the universe.

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44

BENVENUTO, O. G., J. E. HORVATH, and H. VUCETICH. "STRANGE-PULSAR MODELS." International Journal of Modern Physics A 06, no. 27 (November 20, 1991): 4769–830. http://dx.doi.org/10.1142/s0217751x91002276.

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v1.6 We review the theory and observational status of strange-pulsar models. After introduction of the subject, a summary of observational facts about pulsars is presented. The theory of quark matter and strange matter relevant to astrophysical applications is briefly discussed, and applied afterwards to type-II supernova theory and to pulsar models. A discussion of the comparison with observation shows the viability of strange-pulsar models.

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45

Morales‐Barbero, Jennifer, and Julia Vega‐Álvarez. "Input matters matter: Bioclimatic consistency to map more reliable species distribution models." Methods in Ecology and Evolution 10, no. 2 (December 9, 2018): 212–24. http://dx.doi.org/10.1111/2041-210x.13124.

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46

KOMATHIRAJ, K., and S. D. MAHARAJ. "ANALYTICAL MODELS FOR QUARK STARS." International Journal of Modern Physics D 16, no. 11 (November 2007): 1803–11. http://dx.doi.org/10.1142/s0218271807011103.

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We find two new classes of exact solutions to the Einstein–Maxwell system of equations. The matter content satisfies a linear equation of state consistent with quark matter; a particular form of one of the gravitational potentials is specified to generate solutions. The exact solutions can be written in terms of elementary functions, and these can be related to quark matter in the presence of an electromagnetic field. The first class of solutions generalizes the Mak–Harko model. The second class of solutions does not admit any singularities in the matter and gravitational potentials at the center.

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47

Lee, Jae-Weon. "Brief History of Ultra-light Scalar Dark Matter Models." EPJ Web of Conferences 168 (2018): 06005. http://dx.doi.org/10.1051/epjconf/201816806005.

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This is a review on the brief history of the scalar field dark matter model also known as fuzzy dark matter, BEC dark matter, wave dark matter, or ultra-light axion. In this model ultra-light scalar dark matter particles with mass m = O(10-22)eV condense in a single Bose-Einstein condensate state and behave collectively like a classical wave. Galactic dark matter halos can be described as a self-gravitating coherent scalar field configuration called boson stars. At the scale larger than galaxies the dark matter acts like cold dark matter, while below the scale quantum pressure from the uncertainty principle suppresses the smaller structure formation so that it can resolve the small scale crisis of the conventional cold dark matter model.

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48

Atiyah, Michael, and Matilde Marcolli. "Anyon Networks from Geometric Models of Matter." Quarterly Journal of Mathematics 72, no. 1-2 (February 8, 2021): 717–33. http://dx.doi.org/10.1093/qmath/haab004.

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Abstract This paper, completed in its present form by the second author after the first author passed away in 2019, describes an intended continuation of the previous joint work on anyons in geometric models of matter. This part outlines a construction of anyon tensor networks based on four-dimensional orbifold geometries and braid representations associated with surface-braids defined by multisections of the orbifold normal bundle of the surface of orbifold points.

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49

Nagata, Natsumi, Keith A. Olive, and Jiaming Zheng. "Asymmetric dark matter models in SO(10)." Journal of Cosmology and Astroparticle Physics 2017, no. 02 (February 9, 2017): 016. http://dx.doi.org/10.1088/1475-7516/2017/02/016.

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50

Cerdeño, D. G., A. Cheek, E. Reid, and H. Schulz. "Surrogate models for direct dark matter detection." Journal of Cosmology and Astroparticle Physics 2018, no. 08 (August 9, 2018): 011. http://dx.doi.org/10.1088/1475-7516/2018/08/011.

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