Artigos Diversos

[1] Annika H. G. P. Dark Matter, Department of Physics and Astronomy, University of California, Irvine, CA 92697-4575, arXiv:1201.3942v1 [astro-ph.CO] 18 Jan 2012.

[2] Baltz, E. A. Dark Matter Candidates, KIPAC, Stanford University, P.O. Box 20450, MS 29, Stanford, CA 94309, USA. SLAC Summer Institute on Particle Physics (SSI04), Aug. 2-13, 2004.

[3] Bekenstein, J.D. Relativistic gravitation theory for the MOND paradigm, Racah Institute of Physics, Hebrew University of Jerusalem, Givat Ram, Jerusalem 91904 ISRAEL, February 2008.

[4] Bertone, G. and Hooper, D. -A History of Dark Matter, FERMILAB-PUB-16-157-A, arXiv:1605.04909v2 [astro-ph.CO] 24 May 2016. 

[5] Bertone,G. ; Hooper, D. and Silk, J.Particle Dark Matter: Evidence, Candidates and Constraints, FERMILAB-Pub-04/047-A hep-ph/0404175, arXiv:hep-ph/0404175v2 13 Aug 2004. 

[6] Bertone. G. Taoso, M. Masiero, A.Dark Matter Candidates: A Ten-Point Test, Universit´e Pierre et Marie Curie, 98 bis Boulevard Arago 75014, Paris, France, arXiv:0711.4996v2 [astro-ph] 25 Jan 2008. 

[7] Bosma, A., The distribution and kinematics of neutral hydrogen in spiral galaxies of various morphological types, PhD Thesis, Groningen Univ., (1978), Published in 1978 

[8] Baltz, E. A. Dark Matter Candidates, KIPAC, Stanford University, P.O. Box 20450, MS 29, Stanford, CA 94309, USA. SLAC Summer Institute on Particle Physics (SSI04), Aug. 2-13, 2004.

[9] Bosma, A., The distribution and kinematics of neutral hydrogen in spiral galaxies of various morphological types, PhD Thesis, Groningen Univ., (1978), Published in 1978 

[10] Buckley,J., D.F. Cowen, D.F. and S. Profumo, S. Indirect Dark Matter Detection CF2 Working Group Summary, arXiv:1310.7040v1 [astro-ph.HE] 25 Oct 2013.  

[11] Burbidge, E. Margaret, Burbigde G.R, Fowler, Willian A. e Hoyle, F.Synthesis of the Elements in Stars, Reviews of modern physics, volume 29, número 4 outubro de 1957.  

[12] Cardona, S. A. H; Supersimetrial e Modelo Mínimo Supersimetrico, Instituto de Física Teórica, Universidade Estadual Paulista, São Paulo, 2005. 

[13] Carmo, F.M; Um estudo sobre a Supersimetria no contexto da Mecânica Quântica, Instituto de Física; Universidade de São Paulo, São Paulo; 2011. 

[14] Chen, Victor C.; The Micro-Doppler Effect in Radar, Artech House Boston london , 2010. 

[15] Ciotti, l. Londrillo, P. e Nipoti, C.Galaxy merging in MOND, Universidade de Bologna. Itália, 2007. 

[16] Coswik, R. and McClelland, J;Gravity of neutrinos of nonzero mass in Astrophysics, The astrophysical Journal, an international review of spectroscopy and astronaomical physics, vol. 180, pag. 7 – 10, February 1973, 1973ApJ...180....7C. 

[17] Davis, M; Efstathiou, G; Frenk, C. S. and White, S. D. M; The evolution of large-escale structure in a universe dominated by cold dark matter, The astrophysical Journal, an international review of spectroscopy and astronaomical physics, vol. 292, pag. 371 – 394, May 1985, 1985ApJ...292..371D 

[18] Dicke, R. H. The measurement of thermal radiation at microwave frequenciesRev. Sci. Instrum. 17, 268, 1946. 

[19] Dodelson, S. The Real Problem with MOND,Center for Particle Astrophysics, Fermi National Accelerator Laboratory, Batavia, IL 60510 2Department of Astronomy & Astrophysics, The University of Chicago, Chicago, IL 60637 and 3Kavli Institute for Cosmological Physics, Chicago, IL 60637, December 2011.

[20] Drees, M and Gerbier, G. Dark Matter, Bonn University and (Saclay, CEA), Revised September 2013. Disponível emhttp://pdg.lbl.gov/2014/reviews/rpp2014-rev-dark-matter.pdf, acesso janeiro de 2016.

[21] Drukier, A.K. Freese, K. and Spergel D.N. - Detecting cold dark matter candidates, Physical review D, Volume 33, Number 12, June 1986. 

[22] Eduardo Cypriano e Laerte Sodré Jr. A Matéria Escura, April 30, 2009, disponível em:www.astro.iag.usp.br/~laerte/aga5751/dm-wp.pdf, acesso janeiro de 2016.

[23] Eduardo Cypriano, E. Cosmologia com Lentes Gravitacionais Fracas. June 24, 2009. Disponível em:www.astro.iag.usp.br/~laerte/aga5751/lensing-wp.pdf, acesso dezembro de 2015.

[24] Einasto, J. Dark Matter, Tartu Observatory, Estonia, October 20, 2010, arXiv:0901.0632v2 [astro-ph.CO] 19 Oct 2010.

[25] Faber, S.M. and Lin D. N. C; Is there nonluminous matter in dwarf sheroidal Galaxies? The astrophysical Journal, an international review of spectroscopy and astronaomical physics, vol. 266, pag. L17 – L20, March 1983, 1983ApJ...266L..17F.

[26] Fabian, A. C; Thomas, P. A. and White III, R.E; A lower limit binding mass of early-type galaxies, Mon. Not. R. Soc. (1986) vol. 221, page 1049 – 1056, 1986MNRAS.221.1049F

[27] Faria, R. P. -Fundamentos de Astronomia. 3a. ed. Campinas: Papirus, 1987.

[28] Feng. J, e Troden,M. Dark Worlds, A shadow cosmos, woven silently into our own, may have its own rich inner life, Scientific American, pg 40 -45, November 2010.

[29] Feng, J.L. Dark Matter Candidates from Particle Physics and Methods of Detection, Department of Physics and Astronomy, University of California, Irvine, CA 92697, USA  arXiv:1003.0904v2 [astro-ph.CO] 9 Apr 2010.

[30] Fernandes Jr, C. R. Kanaan, A. e Gomes J.M.S.M. -  Observatórios Virtuais – As ferramentas do Astrônomo, o que medimos, como medimos e o que aprendemos (UFSC)

[31] Freeman, K.C, On the disks of spiral and so galaxies, The Asrophysical Journal, vol. 160, june 1970.

[32] Haag, R.; Sohnius, Martin; L., Jan T."All possible generators of supersymmetries of the S-matrix", Nuclear Physics B 88: 257–274, 1975.

[33] Ho-Kim, Q, Kurnar, N and Lam, C.S,Invitation to Contemporary physics, 2nd edition, World Scientific Publishing Co. Pte. Ltd.2004.

[34] Joachim Kopp, J. New signals in dark matter detectors, Fermilab, PO Box 500, Batavia, IL 60510, USA and Max Planck Institut fur Kernphysik, Postfach 10 39 80, 69029 Heidelberg, Germany.

[35] Jones, M. H.; Lambouurne, R. J.A.; SERJEANT, M.K. S.; An Introduction to Galaxies and Cosmology, The Open University, Manchester, 2015.

[36] Jullo, E, Natarajan, P. Kneib,J.P. D’Aloisio, A. Limousin, M. Richard, J. and Schimd, C. - Cosmological Constraints from Strong Gravitational Lensing in Clusters of Galaxies, Science. 2010 Aug 20;329(5994):924-7. doi: 10.1126/science.1185759

[37] Kahn, F. D. and Woltjer, L;Intergalactic matter and the Galaxy, The astrophysical Journal, an international review of spectroscopy and astronaomical physics, vol. 130, n°3, october 1959. 1959ApJ...130..705K.

[38] Kochanek, C.S, The Saas Fee Lectures on Strong Gravitational Lensing, Department of Astronomy, The Ohio State University, arXiv:astro-ph/0407232v1 12 Jul 2004.

[39] Lang, R.F. Ups and Downs in the Search for Dark Matter, Department of Physics, Purdue University, West Lafayette, IN 47907, USA, Published December 16, 2013, American Physical Society, DOI: 10.1103/Physics.6.136.

[40] Linden, T.R. Dark Matter Annihilation at the Galactic Center, University of California, Santa Cruz, USA, June 2013.

[41] Livio, M. ando Silk, J. Broaden the search for dark matter, Macmillan Publishers Limited, Nature, March 2014, Vol. 507, page. 29 a 31.

[42] Longair, M. S. Galaxy formation. 2. ed. Berlin: Springer-Verlag, 2008. 735 p. 12, 16, 20, 22.

[43] Lovell,M. R, Frenk,C. S, Eke, V. R., Jenkins, A., Gao, L. and Theuns, T. -The properties of warm dark matter haloes, Mon. Not. R. Astron. Soc. 000, ??–21 (2012) Printed 20 May 2014 (MN LATEX style file v2.2), arXiv:1308.1399v2 [astro-ph.CO] 19 May 2014.

[44] Marcomini, J.A. - Estudo da possibilidade de detecção da material escura no telescópio Cherencov, Universidade de São Paulo, Instituto de Física, São Carlos, 2015.

[45] Marrodán, T.U and Ludwig Rauch, L. Dark matter direct-detection experiments, arXiv:1509.08767v1 [physics.ins-det] 26 Sep 2015, Max-Planck-Institut fur Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany.

[46] Mark R. Lovell, Carlos S. Frenk, Vincent R. Eke, Adrian Jenkins, Liang Gao and Tom Theuns, The properties of warm dark matter haloes, Mon. Not. R. Astron. Soc. 000, ??–21 (2012) Printed 20 May 2014 (MN LATEX style file v2.2), arXiv:1308.1399v2 [astro-ph.CO] 19 May 2014

[47] Meint P. Van Albada and Ad Lagendijk, Observation of Weak Localization of Light in a Random Medium, Phys. Rev. Lett. 55, 2692 – Published 9 December 1985.

[48] Milgrom, M. A Modification of the Newtonian Dynamics as a possible alternative to the hidden mass hypothesis, the Astrophysical Journal, 270: 365-370, July 1983.

[49] Milgrom, M. A Modification of the Newtonian Dynamics: Implications for Galaxies, the Astrophysical Journal, 270: 371-383, July 1983.

[50] Milgrom, M1. and Robert H. Sanders2, R.H. MOND rotation curves of very low mass spiral galaxies1Center for Astrophysics, Weizmann Institute,2Kapteyn Astronomical Institute, Groningen, NL, arXiv:astro-ph/0611494v1 15 Nov 2006.

[51] Moffat, J.W. Modified Gravity Or Dark Matter? Department of Physics, University of Waterloo, Waterloo, Ontario, Canada, arXiv:1101.1935v2 [astro-ph.CO] 29 Mar 2011.

[52] Moreira, M.A; Grandes desafios para o ensino da física na educação contemporânea, Instituto de Física Universidade Federal do Rio Grande do Sul, 2013.

[53] Noam I. Libeskind,, Arianna Di Cintio, Alexander Knebe, Gustavo Yepes, Stefan Gottlober, Matthias Steinmetz, Yehuda Hoffman, Luis A. Martinez-Vaquero, Cold versus Warm Dark Matter simulations of a galaxy group.

[54] Olbrechts, P. The Search for Neutralino Dark Matter with the AMANDA-B10 Detector, Departement Natuurkunde Faculteit Exacte Wetenschappen Vrije Universiteit Brussel.

[55] Ostermann, F. e Cavalcanti, C. J. H;Física moderna e contemporânea no Ensino Médio: Elaboração de material didático em forma de pôster, sobre partículas elementares e interações fundamentais, Instituto de Física UFRGS, Porto Alegre - RS 

[56] Ostermann F. e Moreira, M.A;Anais do VII Encontro de Pesquisa em Ensino de Física, Florianópolis, 2000.

[57] Ostermann, F.e Moreira, M.A. “Física contemporánea en la escuela secundaria: una experiencia en el aula involucrando formación de profesores”. Enseñanza de las Ciencias, Barcelona, 18(3): 391-404, 2000.

[58] Ostermann F. e Moreira, M.A,Investigações em Ensino de Ciências - Instituto de Física, Universidade Federal do Rio Grande do Sul (2000).

[59] Ostriker, J.P. and Peebles, P.J.E; A numerical study of the stability of flattened galaxies: or, can cold Galaxies survive? The astrophysical Journal, an international review of spectroscopy and astronaomical physics, vol. 186, pag. 467 – 480, December 1973, 1973ApJ...186..467O.

[60] Papantonopoulos, E. Modifications of Einstein's Theory of Gravity at Large Distances, Springer, novembro de 2014

[61] Parker, B; Invisible Matter and the Fate of the Universe, drawings by Lori ,Scoffield. Springer Science Business Media, LLC, 1989.

[62] Pearson, J. Generalized Perturbations in Modified Gravity and Dark Energy, Springer Science & Business Media, EUA ,setembro de 2013

[63] Peebles, P.J.E; Primeval adiabatic perturbations: effect of massive neutrinos, The astrophysical Journal, an international review of spectroscopy and astronaomical physics, vol. 258, pag. 415 – 424, July 1982, 1982ApJ...258..415P.

[64] Peter S.; Extragalactic Astronomy and Cosmology An Introduction Springer-Verlag Berlin Heidelberg 2006.

[65] Philip Olbrechts, P. The Search for Neutralino Dark Matter with the AMANDA-B10 Detector, Departement Natuurkunde Faculteit Exacte Wetenschappen Vrije Universiteit Brussel.

[66] Picon, C. A. and Neelakanta, J, T.How Cold is Cold Dark Matter?Department of Physics, Syracuse University, Syracuse, NY 13244-1130, USA, arXiv:1309.6971v2 [astro-ph.CO] 31 Mar 2014

[67] Primack, J. - Historical Introduction to ΛCDM Cosmology, University of California, Santa Cruz, dezembro de 2012. 

[68] Primack, J. - A Brief History of Dark Matter, University of California, Santa Cruz, dezembro de 2012.

[69] Primack , J.R., Dark Matter, Galaxies and large scale structure in the universe, [1] Stanford Linear Accelerator Center, Stanford University, Stanford, California, and Santa Crux Institute of Particle Physics, University of California, Santa Cruz, Lectures presented at the International School of Physics “Enrico Fermi” ,Varenna, Italy, June 26 - July 6, 1984.

[70] Primack, J. R., Dark Matter and Galaxy Formation, Physics Department, University of California, Santa Cruz, CA 95064 USA.

[71] Primack, J. R., Cosmology: small scale issues , Physics Department, University of California, Santa Cruz, CA 95064 USA.

[72] Primack, J. R., The nature of dark matter, Physics Department, University of California, Santa Cruz, CA 95064 USA, Lectures at International School of Space Science, L’Aquila, Italy, August-September 2001, To be published in the Frascati Physics Series by S.I.S.-Laboratori Nazionali di Frascati, arXiv:astro-ph/0112255v2 14 Dec 2001.

[73] Primack, J.R., Flores, R., Blumental, G.R. and Faber, M. Contarction of dark matter galactic halos due to baryonic infall, The Asrophysical Journal, 301: 27-34, 1986, Febuary 1.

[74] Queiroz, F.S. - Detecção Direta e Indireta de Matéria Escura em Teorias de Gauge, Centro de ciências exatas e da Natureza, Universidade federal da Paraíba, 2013.

[75] Ramesh Narayan, R. and Bartelmann, M. Lectures on Gravitational Lensing, Harvard-Smithsonian Center for Astrophysics and Max-Planck-Institut f¨ur Astrophysik, 2011.

[76] Rees, M. 1977, In The Evolution of Galaxies and Stellar Populations, Eds. B.M. Tinsley and R.B. Larson (New Haven: Yale Univ. Observatory), p. 339 

[77] Reich, E.S. Dark matter hunt gets deep - China launches world’s deepest particle-physics experiment — but it joins a crowded field. Macmillan Publishers Limited, Nature, February, Vol 494, page 291 a 292.

[78] Reich, E.S Final word is near on dark-matter signal - An influential US experiment prepares to release its first results, Macmillan Publishers Limited, Nature, October 2013, Vol 502, page 421.

[79] Rubin, V.C. and Ford, K. W; Rotation of the Andromeda nebula from a spectroscopic survey os emission regions, The astrophysical Journal, an international review of spectroscopy and astronaomical physics, vol. 159, n°3, February 1970. 1970ApJ...159..379R.

[80] Rubin, V.C Ford. Jr W.K, and Thonnard, N. Rotacional properties of 21 Sc galaxies with a large range of luminisities and radII, from NGC 4605 (R=4Kpc) to UCG 2885 (R=122 kpc), The Asrophysical Journal, 238: 471-487, 1980, june 1.

[81] Sanders, R.H. Forming galaxies with MOND, Kapteyn Astronomical Institute, P.O. Box 800, 9700 AV Groningen, The Netherlands, February 2013.

[82] Sanders, R.H. and Noordermeer, E.2,Confrontation of MOND with the rotation curves of early-type disc galaxies1Kapteyn Astronomical Institute, University of Groningen, P.O. Box 800, 9700 AV Groningen, The Netherlands, 2University of Nottingham, School of Physics and Astronomy, University Park, NG7 2RD Nottingham, UK, arXiv:astro-ph/0703352v1 14 Mar 2007.

[83] Scott & Smoot, Cosmic Microwave Background, cap. 25, livro Particle Data Group 2012 (pdg.lbl.gov) 

http://map.gsfc.nasa.gov/ visitado em setembro de 2015 

[84] Shigetaka Moriyama, S., Direct Detection of Dark Matter,Kamioka Observatory, Institute of Cosmic Ray Research, the University of Tokyo, Kamioka cho, Hida city, Gifu prefecture, Japan.

[85] Sigurdson, K., Hidden Hot Dark Matter as Cold Dark Matter, Kris Sigurdson Department of Physics and Astronomy, University of British Columbia, Vancouver, BC V6T 1Z1, Canada, 2009.

[86] Silva, L.J.B. Sinais experimentais de matéria escura supermassiva fortemente interagente, Instituto de Física da Universidade de São Paulo, São Paulo, 2010.

[87] Sinziana Paduroiu, S., Revaz, Y.,Pfenniger, D. - Structure formation in warm dark matter cosmologies Top-Bottom Upside-Down, Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 24 June 2015 (MN LATEX style file v2.2), arXiv:1506.03789v2 [astro-ph.CO] 23 Jun 2015.

[88] Sohnius, M. F. - Introducing Supersymmetry Physics Reports, 128, Nos 2 & 3, pp. 39-204, 1985.

[89] Sotelo, D.S.R. Testes de modelos de matéria escura relacionados aos excessos leptônicos medidos por PAMELA e FermiLAT, Universidade de São Paulo, Instituto de Física, São Paulo, 2012.

[90] Spano M., Marcelin M., Amram, P., Carignan C., Epinat B., Hernandez O., GHASP : an Hα kinematic survey of spiral and irregular galaxies. V. Dark matter distribution in 36 nearby spiral galaxies, arXiv:0710.1345v1 [astro-ph] 6 Oct 2007

[91] Sparke, L..; Gallanger, S. e Jonh S. Galaxies in the Universe, An Introduction; University of Wisconsin, Madison 2007. 

[92] Stwart, G. C; Fabian, A. C; Jones, C. and Forman, W; The prevalence of cooling flows in clusters of Galaxies, The astrophysical Journal, an international review of spectroscopy and astronaomical physics, vol. 285, pag. 1 – 6, October 1984, 1984ApJ...285....1S.

[93] Tiret, O. and Combes, F. Interacting Galaxies with MOND, Observatoire de Paris, LERMA, 2007.

[94] Tongyan, L. Signals of Particle Dark Matter, Doctoral dissertation, Harvard University, 2012.

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[96] Van Den Bergh, S. - THE EARLY HISTORY OF DARK MATTER, Dominion Astrophysical Observatory Herzberg Institute of Astrophysics National Research Council of Canada, astro-ph/9904251 19 Apr 1999.

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[98] Viel, M., Becker, G. D., Bolton, J.S, G. Haehnel, M.G - Warm Dark Matter as a solution to the small scale crisis: new constraints from high redshift Lyman-α forest data,arXiv:1306.2314v2 [astro-ph.CO] 26 Aug 2013 

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