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Journal articles on the topic 'Dark matter'

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Author: Grafiati

Published: 4 June 2021

Last updated: 31 July 2024

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1

R K Dubey, R. K. Dubey, Pratima Ojha, and Anil Saini. "Cosmological Model with Dark Energy and Dark Matter." International Journal of Scientific Research 2, no. 5 (June 1, 2012): 400–401. http://dx.doi.org/10.15373/22778179/may2013/135.

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2

Perković, Dalibor, and Hrvoje Štefančić. "Dark sector unifications: Dark matter-phantom energy, dark matter - constant w dark energy, dark matter-dark energy-dark matter." Physics Letters B 797 (October 2019): 134806. http://dx.doi.org/10.1016/j.physletb.2019.134806.

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3

Nadar, Arun Kumar Koottharasan. "Exploring the Nature of Dark Matter and Dark Energy." International Journal of Research Publication and Reviews 5, no. 1 (January 24, 2024): 4640–46. http://dx.doi.org/10.55248/gengpi.5.0124.0341.

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4

Hogan, Craig J. "Dark dark matter." Nature 351, no. 6322 (May 1991): 96–97. http://dx.doi.org/10.1038/351096b0.

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5

Olive, Keith A. "Dark matter and dark matter candidates." Advances in Space Research 42, no. 3 (August 2008): 581–90. http://dx.doi.org/10.1016/j.asr.2007.07.040.

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6

Edmonds, Douglas, Duncan Farrah, Djordje Minic, Y. Jack Ng, and Tatsu Takeuchi. "Modified dark matter: Relating dark energy, dark matter and baryonic matter." International Journal of Modern Physics D 27, no. 02 (January 2018): 1830001. http://dx.doi.org/10.1142/s021827181830001x.

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Modified dark matter (MDM) is a phenomenological model of dark matter, inspired by gravitational thermodynamics. For an accelerating universe with positive cosmological constant ([Formula: see text]), such phenomenological considerations lead to the emergence of a critical acceleration parameter related to [Formula: see text]. Such a critical acceleration is an effective phenomenological manifestation of MDM, and it is found in correlations between dark matter and baryonic matter in galaxy rotation curves. The resulting MDM mass profiles, which are sensitive to [Formula: see text], are consistent with observational data at both the galactic and cluster scales. In particular, the same critical acceleration appears both in the galactic and cluster data fits based on MDM. Furthermore, using some robust qualitative arguments, MDM appears to work well on cosmological scales, even though quantitative studies are still lacking. Finally, we comment on certain nonlocal aspects of the quanta of modified dark matter, which may lead to novel nonparticle phenomenology and which may explain why, so far, dark matter detection experiments have failed to detect dark matter particles.

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7

Poojary, Bhushan. "Dark Matter and Quantum Entanglement Decoded." International Journal of Applied Physics and Mathematics 4, no. 3 (2014): 180–83. http://dx.doi.org/10.7763/ijapm.2014.v4.279.

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8

Battersby, Stephen. "Dark matter, dark energy, dark… magnetism?" New Scientist 214, no. 2867 (June 2012): 36–39. http://dx.doi.org/10.1016/s0262-4079(12)61430-4.

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9

de la Macorra, A. "Dark group: dark energy and dark matter." Physics Letters B 585, no. 1-2 (April 2004): 17–23. http://dx.doi.org/10.1016/j.physletb.2004.02.006.

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10

MORIYAMA, Shigetaka. "Dark Matter." RADIOISOTOPES 63, no. 3 (2014): 151–62. http://dx.doi.org/10.3769/radioisotopes.63.151.

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11

Vlček, Martin. "Dark matter." American Journal of Biomedical Science & Research 9, no. 6 (August 26, 2020): 54–55. http://dx.doi.org/10.34297/ajbsr.2020.10.001473.

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12

Buckley, Christopher. "Dark Matter." Iowa Review 20, no. 2 (April 1990): 50–51. http://dx.doi.org/10.17077/0021-065x.3882.

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13

Susanne Antonetta. "Dark Matter." Fourth Genre: Explorations in Nonfiction 15, no. 1 (2013): 59. http://dx.doi.org/10.14321/fourthgenre.15.1.0059.

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14

Williams, John Alfred. "Dark Matter." Callaloo 30, no. 3 (2007): 884–88. http://dx.doi.org/10.1353/cal.2008.0011.

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15

Baker, Aaron. "Dark Matter." Missouri Review 36, no. 2 (2013): 94. http://dx.doi.org/10.1353/mis.2013.0058.

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16

Emma Fuller. "Dark Matter." Framework: The Journal of Cinema and Media 54, no. 1 (2013): 108. http://dx.doi.org/10.13110/framework.54.1.0108.

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17

McGaw, Janet. "Dark Matter." Architectural Theory Review 22, no. 1 (January 2, 2018): 120–39. http://dx.doi.org/10.1080/13264826.2018.1413406.

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18

SPERGEL, DAVID N. "Dark Matter." Annals of the New York Academy of Sciences 571, no. 1 Texas Symposi (December 1989): 298–307. http://dx.doi.org/10.1111/j.1749-6632.1989.tb50517.x.

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19

Mole. "Dark matter." Journal of Cell Science 123, no. 21 (October 21, 2010): 3617–18. http://dx.doi.org/10.1242/jcs.080317.

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20

Peebles, P. James E. "Dark matter." Proceedings of the National Academy of Sciences 112, no. 40 (May 2, 2014): 12246–48. http://dx.doi.org/10.1073/pnas.1308786111.

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The evidence for the dark matter (DM) of the hot big bang cosmology is about as good as it gets in natural science. The exploration of its nature is now led by direct and indirect detection experiments, to be complemented by advances in the full range of cosmological tests, including judicious consideration of the rich phenomenology of galaxies. The results may confirm ideas about DM already under discussion. If we are lucky, we also will be surprised once again.

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21

Sancisi, R., and T. S. van Albada. "Dark Matter." Symposium - International Astronomical Union 124 (1987): 699–712. http://dx.doi.org/10.1017/s0074180900159807.

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The observational evidence for unseen matter is briefly reviewed for objects ranging from small to very large scales. The existence of large mass discrepancies is clearly recognized in individual spiral galaxies and in rich clusters of galaxies. For other systems - dwarfs, ellipticals, binaries and groups - the results are more uncertain and still rather controversial. The data on spirals indicate values of the cosmological density parameter Ω around 0.02, those on clusters Ω ≃ 0.2. The spatial distribution of this dark matter is still largely unknown: while on the galaxy scale it must be located mainly in the outer parts of the stellar system, in clusters it is unclear whether it follows the distribution of the visible galaxies or not.

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22

Einasto, Jaan. "Dark Matter." Brazilian Journal of Physics 43, no. 5-6 (June 27, 2013): 369–74. http://dx.doi.org/10.1007/s13538-013-0147-9.

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23

Spergel, David N. "Dark matter." Nuclear Physics B - Proceedings Supplements 13 (February 1990): 66–74. http://dx.doi.org/10.1016/0920-5632(90)90038-v.

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24

Fuller, Emma. "Dark Matter." Framework: The Journal of Cinema and Media 54, no. 1 (2013): 108–10. http://dx.doi.org/10.1353/frm.2013.0007.

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25

Antonetta, Susanne. "Dark Matter." Fourth Genre: Explorations in Nonfiction 15, no. 1 (2013): 59–63. http://dx.doi.org/10.1353/fge.2013.0482.

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26

GREEN, S. "Dark Matter." Science 255, no. 5046 (February 14, 1992): 858–59. http://dx.doi.org/10.1126/science.255.5046.858-a.

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27

Lincoln, Don. "Dark Matter." Physics Teacher 51, no. 3 (March 2013): 134–38. http://dx.doi.org/10.1119/1.4792003.

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28

Höfler, Stefan. "Dark Matter." Indo-European Linguistics 3, no. 1 (2015): 24–41. http://dx.doi.org/10.1163/22125892-00301004.

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The assumption of a root *√k̑u̯el ‘dark, black’ offers new possible etymologies for Arm. šaɫax, Gk. πηλός, Toch. B kwele, Hitt. kuu̯aliu-, Gk. κύλα, Lat. culex, and Lat. color, whose derivational background will be dealt with in the course of this paper.

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29

Ramachers, Yorck. "Dark Matter." Europhysics News 32, no. 6 (November 2001): 242–44. http://dx.doi.org/10.1051/epn:2001615.

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30

Moore, Ben. "Dark matter." Philosophical Transactions of the Royal Society of London. Series A: Mathematical, Physical and Engineering Sciences 357, no. 1763 (December 1999): 3259–76. http://dx.doi.org/10.1098/rsta.1999.0493.

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31

Mani, P. Seshu. "Dark Matter." International Journal of Agriculture & Environmental Science 6, no. 2 (March 25, 2019): 78–82. http://dx.doi.org/10.14445/23942568/ijaes-v6i2p115.

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32

Marcum, Carl. "[ Dark Matter ]." Pleiades: Literature in Context 40, no. 1 (2020): 127–28. http://dx.doi.org/10.1353/plc.2020.0038.

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33

Srednicki, M. "Dark Matter." European Physical Journal C 15, no. 1-4 (March 2000): 143–44. http://dx.doi.org/10.1007/bf02683414.

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34

Spiro, Michel. "Dark matter." Nuclear Physics B - Proceedings Supplements 43, no. 1-3 (June 1995): 100–107. http://dx.doi.org/10.1016/0920-5632(95)00460-q.

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35

Phookun, Bikram, and Biman Nath. "Dark matter." Resonance 4, no. 9 (September 1999): 24–31. http://dx.doi.org/10.1007/bf02834229.

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36

Phookun, Bikram, and Biman Nath. "Dark matter." Resonance 4, no. 10 (October 1999): 40–46. http://dx.doi.org/10.1007/bf02834258.

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37

Phookun, Bikram, and Biman Nath. "Dark matter." Resonance 10, no. 12 (December 2005): 76–82. http://dx.doi.org/10.1007/bf02835131.

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38

Ginn, Stephen. "Dark matter." Lancet 402, no. 10400 (August 2023): 443. http://dx.doi.org/10.1016/s0140-6736(23)01578-7.

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39

Burkert, A. "Fuzzy Dark Matter and Dark Matter Halo Cores." Astrophysical Journal 904, no. 2 (November 30, 2020): 161. http://dx.doi.org/10.3847/1538-4357/abb242.

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40

常, 炳功. "Matter-Dark Matter-Dark Energy Are a Whole." Modern Physics 08, no. 05 (2018): 239–52. http://dx.doi.org/10.12677/mp.2018.85026.

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41

Xu, Chongming, and Xuejun Wu. "To Solve Dark Matter Problems Without Dark Matter." Symposium - International Astronomical Union 201 (2005): 534–35. http://dx.doi.org/10.1017/s0074180900217014.

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42

Regmi, Jeevan. "Dark Energy and Dark Matter." Himalayan Physics 4 (December 23, 2013): 91–94. http://dx.doi.org/10.3126/hj.v4i0.9436.

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The new discoveries and evidences in the field of astrophysics have explored new area of discussion each day. It provides an inspiration for the search of new laws and symmetries in nature. One of the interesting issues of the decade is the accelerating universe. Though much is known about universe, still a lot of mysteries are present about it. The new concepts of dark energy and dark matter are being explained to answer the mysterious facts. However it unfolds the rays of hope for solving the various properties and dimensions of space.The Himalayan Physics Vol. 4, No. 4, 2013 Page: 90-94 Uploaded date: 12/23/2013

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43

Caldwell, Robert, and Marc Kamionkowski. "Dark matter and dark energy." Nature 458, no. 7238 (April 2009): 587–89. http://dx.doi.org/10.1038/458587a.

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44

Comelli, D., M. Pietroni, and A. Riotto. "Dark energy and dark matter." Physics Letters B 571, no. 3-4 (October 2003): 115–20. http://dx.doi.org/10.1016/j.physletb.2003.05.006.

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45

Khuri, Ramzi R. "Dark matter as dark energy." Physics Letters B 568, no. 1-2 (August 2003): 8–10. http://dx.doi.org/10.1016/j.physletb.2003.06.051.

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46

Eckhardt, Donald H., and José Luis Garrido Pestaña. "Dark Future for Dark Matter." Journal of Modern Physics 11, no. 10 (2020): 1589–97. http://dx.doi.org/10.4236/jmp.2020.1110099.

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47

Wu, Yumiao. "The dark matter and dark energy." SHS Web of Conferences 174 (2023): 03014. http://dx.doi.org/10.1051/shsconf/202317403014.

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The dark matter and dark energy are one of the biggest challenges facing contemporary physics and astronomy. Dark energy and dark matter play an important role the universe. The amount of dark energy and dark matter determines how the universe changes. When there’s more dark energy, the universe is accelerating. If there were more dark matter, the universe might slow down, or even stop expanding and start contracting. So in this paper, the basic definition of dark matter and dark energy are introduced. And how were dark matter and dark energy discovered and their respective detection methods and the current progress of experiments to detect dark matter and dark energy respectively.

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48

Wang, Huai-Yu. "A theory of dark energy that matches dark matter." Physics Essays 36, no. 2 (June 27, 2023): 149–59. http://dx.doi.org/10.4006/0836-1398-36.2.149.

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In this paper, a theory of dark energy is proposed that matches dark matter. The relativistic quantum mechanics equations reveal that free particles can have negative energies. We think that the negative energy is the dark energy, which behaves as dark photons with negative energies. In this work, the photon number states are extended to the cases where the photon number can be negative integers, called negative integer photon states, the physical meaning of which are that the photons in such a state are of negative energy, i.e., dark photons. The dark photons constitute dark radiation, also called negative radiation. The formalism of the statistical mechanics and thermodynamics of the dark radiation is presented. This version of dark energy is of negative temperature and negative pressure, the latter regarded as responsible for the accelerate expansion of the universe. It is believed that there is a symmetry of energy-dark energy in the universe. In our previous work, the theory of the motion of the matters with negative kinetic energy was presented. In our opinion, the negative kinetic energy matter is dark matter. In the present work, we demonstrate that the dark substances absorb and release dark energy. In this view, the dark matter and dark energy match. Therefore, there is a symmetry of matter-energy match and dark matter-dark energy match in the universe. We present the reasons why the negative kinetic energy systems and negative radiation are dark to us.

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49

Chang, Yi-Fang. "Negative Matter as Unified Dark Matter and Dark Energy, Distributions of Dark Matter-Energy, and Observed Ways in the Milky Way." European Journal of Theoretical and Applied Sciences 1, no. 6 (November 1, 2023): 399–410. http://dx.doi.org/10.59324/ejtas.2023.1(6).39.

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There are not necessarily dark matter and dark energy in the solar system, and dark energy cannot distribute uniformly in the whole space. Based on Dirac negative energy, Einstein mass-energy relation and principle of equivalence, we proposed the negative matter as the simplest model of unified dark matter and dark energy. All theories are known, only mass includes positive and negative. Because there is repulsion between positive matter and negative matter, so which is invisible dark matter, and repulsion as dark energy. It may explain many phenomena of dark matter and dark energy. We derive that the rotational velocity of galaxy is approximate constant, and an evolutional ratio between total matter and usual matter from 1 to present 11.82 or 7.88. We calculate the accelerated expansion at 9.760 billion years. Further, the mechanism of inflation is origin of positive-negative matters created from nothing, whose expansion is exponential due to strong interactions at small microscopic scales. We propose specifically some possible ways on observe dark matter in the Milky Way. Many observatories should be able to observe these results. Final, we research some basic problems in cosmology: Possible mechanism of missing antimatter, the origins of mass and charge, etc. The negative matter as a candidate of unified dark matter and dark energy is not only the simplest, and is calculable, observable and testable, and may be changed and developed.

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50

Burghardt, Rainer. "Dark Matter without Matter." Journal of Modern Physics 09, no. 13 (2018): 2320–41. http://dx.doi.org/10.4236/jmp.2018.913147.

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