Bibliografias temáticas / Missing mass (Astronomy)

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Literatura científica selecionada sobre o tema "Missing mass (Astronomy)"

Autor: Grafiati
Publicado: 4 de junho de 2021
Última modificação: 31 de janeiro de 2023

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Artigos de revistas sobre o assunto "Missing mass (Astronomy)"

1

Malkov, O. Yu. "Local missing mass." Astrophysics 37, no. 3 (July 1994): 256–60. http://dx.doi.org/10.1007/bf02058781.

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Visser, Matt. "Is the ?missing mass? really missing?" General Relativity and Gravitation 20, no. 1 (January 1988): 77–81. http://dx.doi.org/10.1007/bf00759258.

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Atkins, Chris. "The missing mass." Physics World 34, no. 10 (December 1, 2021): 25v. http://dx.doi.org/10.1088/2058-7058/34/10/32.

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In response to the Lateral Thoughts quiz “Sporting chance”, in which question 8 asked for a rough estimate of the theoretical maximum height a pole vaulter could jump, and why the actual world record is slightly above this.
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Petit, J. P. "The missing-mass problem." Il Nuovo Cimento B 109, no. 7 (July 1994): 697–709. http://dx.doi.org/10.1007/bf02722527.

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Krishan, V. "Rotation curves of galaxies: Missing mass or missing physics." Pramana 49, no. 1 (July 1997): 147–54. http://dx.doi.org/10.1007/bf02856345.

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Schatzman, E. "Missing mass or dark matter?" International Journal of Theoretical Physics 28, no. 9 (September 1989): 1169–71. http://dx.doi.org/10.1007/bf00670357.

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Surdin, M. "The Missing Mass of the Universe." Physics Essays 13, no. 1 (March 2000): 130–31. http://dx.doi.org/10.4006/1.3025419.

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Trippe, Sascha. "The ‘Missing Mass Problem’ in Astronomy and the Need for a Modified Law of Gravity." Zeitschrift für Naturforschung A 69, no. 3-4 (April 1, 2014): 173–87. http://dx.doi.org/10.5560/zna.2014-0003.

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Since the 1930s, astronomical observations have accumulated evidence that our understanding of the dynamics of galaxies and groups of galaxies is grossly incomplete: assuming the validity of Newton’s law of gravity on astronomical scales, the observed mass (stored in stars and interstellar gas) of stellar systems can account only for roughly 10% of the dynamical (gravitating) mass required to explain the high velocities of stars in those systems. The standard approach to this ‘missing mass problem’ has been the postulate of ‘dark matter’, meaning an additional, electromagnetically dark, matter
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Gorjup, Niko, and Amrit Sorli. "SMBH relativistic mass and missing dark matter." Advanced Studies in Theoretical Physics 16, no. 4 (2022): 291–97. http://dx.doi.org/10.12988/astp.2022.91963.

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Cook, Richard I., and I. P. Dell'Antonio. "THE MISSING WEAK LENSING MASS IN A781." Astrophysical Journal 750, no. 2 (April 25, 2012): 153. http://dx.doi.org/10.1088/0004-637x/750/2/153.

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Teses / dissertações sobre o assunto "Missing mass (Astronomy)"

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Ng, Shao-Chin Cindy. "Cosmological models with quintessence : dynamical properties and observational constraints." Title page, table of contents and abstract only, 2001. http://web4.library.adelaide.edu.au/theses/09PH/09phn5758.pdf.

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Bibliography: leaves 100-106. Studies different models of "quintessence", in particular, a quintessence arising from an ultra-light pseudo Nambu-Goldstone boson. Overviews dynamical properties for these models using phase-space analyses to study attractor and tracker solutions. Studies high-redshift type Ia supernovae constraints on these models. Studies the impact of a simple phenomenological model for supernovae luminosity evolution on the PNGB models and the potentials of a future supernovae data set to discriminate the PNGB models over the other quintessence models. Studies gravitational l
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2

Bebronne, Michael. "Theoretical and phenomenological aspects of theories with massive gravitons." Doctoral thesis, Universite Libre de Bruxelles, 2009. http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/210253.

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Depuis sa formulation au début du 20ème siècle, la théorie de la Relativité Générale a été vérifiée avec une précision sans cesse croissante. Cette théorie prédit, entre autre, l'existence d'ondes gravitationnelles qui restent à ce jour inobservées, et ce malgré de nombreuses tentatives de détections. Ces ondes sont caractérisées par leur absence de masse. Une des questions qui se pose alors est de savoir si cette absence de masse est une condition nécessaire pour que théorie et observations concordent. Pour répondre à cette question, il est indispensable d'étudier les différents aspects des t
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Capela, Fabio. "Black holes and the dark sector." Doctoral thesis, Universite Libre de Bruxelles, 2014. http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/209310.

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This thesis is divided in two parts: the first part is dedicated to the study of black hole solutions in a theory of modified gravity, called massive gravity, that may be able to explain the actual stage of accelerated expansion of the Universe, while in the second part we focus on constraining primordial black holes as dark matter candidates.<p><p>In particular, during the first part we study the thermodynamical properties of specific black hole solutions in massive gravity. We conclude that such black hole solutions do not follow the second and third of law of thermodynamics, which may signa
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Ng, Shao-Chin Cindy. "Cosmological models with quintessence : dynamical properties and observational constraints / Shao-Chin Cindy Ng." Thesis, 2001. http://hdl.handle.net/2440/21740.

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Bibliography: leaves 100-106.<br>v, 107 leaves : ill. ; 30 cm.<br>Studies different models of "quintessence", in particular, a quintessence arising from an ultra-light pseudo Nambu-Goldstone boson. Overviews dynamical properties for these models using phase-space analyses to study attractor and tracker solutions. Studies high-redshift type Ia supernovae constraints on these models. Studies the impact of a simple phenomenological model for supernovae luminosity evolution on the PNGB models and the potentials of a future supernovae data set to discriminate the PNGB models over the other quintess
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Schmidt, Ralph [Verfasser]. "Automatische Bestimmung von Verknüpfungspunkten für HRSC-Bilder der Mars Express-Mission / von Ralph Schmidt." 2008. http://d-nb.info/991013719/34.

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Pauly, Kristian [Verfasser]. "In situ consumable production for Mars missions / Kristian Pauly." 2002. http://d-nb.info/967531640/34.

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Livros sobre o assunto "Missing mass (Astronomy)"

1

Mass and matter. Mankato, MN: Creative Education, 2012.

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2

Krauss, Lawrence Maxwell. Quintessence: The mystery of missing mass in the universe. New York: Basic Books, 2000.

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3

Tucker, Wallace H. The dark matter: Contemporary science's quest for the mass hidden in our universe. New York: Morrow, 1988.

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4

Hawkins, Michael. Hunting down the universe: The missing mass, primordial black holes, and other dark matters. Reading, Mass: Addison-Wesley, 1997.

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5

Michael, Hawkins. Hunting down the universe: The missing mass, primordial black holes, and other dark matters. London: Little, Brown, 1997.

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6

Celia, Fitzgerald, ed. Hunting down the universe: The missing mass, primordial black holes, and other dark matters. Reading, Mass: Perseus Books, 1998.

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7

Gribbin, John R. The Omega Point: The search for the missing mass and the ultimate fate of the universe. Toronto: Bantam Books, 1988.

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8

Gribbin, John R. The Omega Point: The search for the missing mass and the ultimate fate of the universe. London: Heinemann, 1987.

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9

Papantonopoulos, E. The invisible universe: Dark matter and dark energy. [New York]: Springer-Verlag Berlin Heidelberg, 2010.

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10

The hidden universe. New York: E. Horwood, 1991.

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Capítulos de livros sobre o assunto "Missing mass (Astronomy)"

1

Rothenflug, R., and M. Arnaud. "Galaxy Clusters: The Missing Mass in Stars." In X-Ray Astronomy in the Exosat Era, 689–92. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5448-9_96.

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Trabalhos de conferências sobre o assunto "Missing mass (Astronomy)"

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Rouverand, Léa, Cerise Cuny, Elena López-Contreras González, Marine Prunier, Mathéo Fouchet, Nicolas Wattelle, Valentine Bourgeois, Quentin Royer, and Marie Delaroche. "Experiment collaboration program during a Martian analogue mission to introduce young students to human space exploration." In Symposium on Space Educational Activities (SSAE). Universitat Politècnica de Catalunya, 2022. http://dx.doi.org/10.5821/conference-9788419184405.090.

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The last decade has demonstrated an increased public and private interest towards crewed missions through the emergence of New Space and the Artemis program. There is therefore a need to form the next generation of scientists to prepare future crewed space exploration missions. In this context, it is important to familiarize teenagers with the scientific issues of today’s world and to inspire them to engage in the space sector. Crew 263 is a group of seven students preparing a Martian analogue mission at the Mars Desert Research Station (MDRS) in the desert of Utah (United States). A Martian a
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2

Cherepashchuk, A. M., T. S. Khruzina, and A. I. Bogomazov. "Parameters of Sco X-1." In ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES. Proceedings of the VAK-2021 conference, Aug 23–28, 2021. Crossref, 2022. http://dx.doi.org/10.51194/vak2021.2022.1.1.039.

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We modelled optical light curves of Sco X-1 obtained by the Kepler K2 mission. We calculated the ratio of the mass of therelativistic object to the mass of the optical star q = M x /M v = 3.6 (3.5 − 3.8) and the orbital inclination i = 30 ◦ (25 ◦ − 34 ◦ ).
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Fleming, Brian T., Kevin C. France, Nicholas Nell, Richard A. Kohnert, Keri Hoadley, Pascal M. Petit, Aline A. Vidotto, et al. "The Colorado Ultraviolet Transit Experiment (CUTE): a dedicated cubesat mission for the study of exoplanetary mass loss and magnetic fields." In UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XX, edited by Oswald H. Siegmund. SPIE, 2017. http://dx.doi.org/10.1117/12.2276138.

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Ueta, Toshiya, Hideyuki Izumiura, Issei Yamamura, Osamu Hashimoto, Mikako Matsuura, Takashi Miyata, Yoshikazu Nakada, et al. "Excavating Mass Loss History in Extended Dust Shells of Evolved Stars: the MLHES Mission Programme with the AKARI Astronomy Satellite." In UNSOLVED PROBLEMS IN STELLAR PHYSICS: A Conference in Honor of Douglas Gough. AIP, 2007. http://dx.doi.org/10.1063/1.2818995.

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