Literatura académica sobre el tema "Q-stars"
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Artículos de revistas sobre el tema "Q-stars"
Lynn, Bryan W. "Q-stars". Nuclear Physics B 321, n.º 2 (julio de 1989): 465–80. http://dx.doi.org/10.1016/0550-3213(89)90352-0.
Texto completoBahcall, Safi, Bryan W. Lynn y Stephen B. Selipsky. "Are neutron stars Q-stars?" Nuclear Physics B 331, n.º 1 (febrero de 1990): 67–79. http://dx.doi.org/10.1016/0550-3213(90)90018-9.
Texto completoBahcall, Safi, Bryan W. Lynn y Stephen B. Selipsky. "Fermion Q-stars". Nuclear Physics B 325, n.º 3 (octubre de 1989): 606–18. http://dx.doi.org/10.1016/0550-3213(89)90498-7.
Texto completoSelipsky, Stephen B., Dallas C. Kennedy y Bryan W. Lynn. "Non-abelian Q-stars". Nuclear Physics B 321, n.º 2 (julio de 1989): 430–38. http://dx.doi.org/10.1016/0550-3213(89)90350-7.
Texto completoBecerril, R., A. Bernal, F. S. Guzmán y U. Nucamendi. "Stability properties of Q-stars". Physics Letters B 657, n.º 4-5 (diciembre de 2007): 263–68. http://dx.doi.org/10.1016/j.physletb.2007.07.077.
Texto completoSu, Ru-Keng, Cheng-Gang Su y Rong-Shi Pan. "Q-stars at finite temperature". Physics Letters B 278, n.º 3 (marzo de 1992): 297–301. http://dx.doi.org/10.1016/0370-2693(92)90196-b.
Texto completoPrikas, Athanasios. "Q-stars in 2+1 dimensions". Nuclear Physics B 690, n.º 3 (julio de 2004): 201–29. http://dx.doi.org/10.1016/j.nuclphysb.2004.05.005.
Texto completoGeng, Yuan-Yuan, Dong-Nuan Cui, Jiang Zhang y Bo Zhang. "Exploring the nucleosynthesis region of metal-poor Stars". Proceedings of the International Astronomical Union 4, S252 (abril de 2008): 339–40. http://dx.doi.org/10.1017/s1743921308023144.
Texto completoPrikas, Athanasios. "Q-Stars in Anti de Sitter Spacetime". General Relativity and Gravitation 36, n.º 8 (agosto de 2004): 1841–69. http://dx.doi.org/10.1023/b:gerg.0000035955.07614.0d.
Texto completoMadsen, Jes. "Detecting supersymmetric Q-balls with neutron stars". Physics Letters B 435, n.º 1-2 (septiembre de 1998): 125–30. http://dx.doi.org/10.1016/s0370-2693(98)00789-8.
Texto completoTesis sobre el tema "Q-stars"
Pombo, Alexandre Mira. "Q-ball spectroscopy and construction of boson stars". Master's thesis, Universidade de Aveiro, 2017. http://hdl.handle.net/10773/23513.
Texto completoNa ausência de efeitos gravitacionais, a dispersão da equação linear de Klein- Gordon pode ser contrabalan cada pela introdução de auto-interações não-lineares do campo escalar. Quando ocorre o cancelamento de efeitos não lineares e dispersivos, ocorrem pacotes auto-reforçadas de ondas solitárias. Quando um único campo escalar complexo produz soluções solit onicas, eles são conhecidos como Qballs. O tipo mais genérico de Q-balls possui uma rotação e uma carga elétrica e são denominados \gauged, spinning Q-balls". Nesta tese, após uma breve introdução do modelo e algumas propriedades físicas e assintóticas, um método espectroscópico para decompor os vários campos das Q-ball e introduzido e os vários modos obtidos a partir dele são analisados. De modo a analisar estes, algumas quantidades físicas são estudadas e comparadas entre as diferentes soluções de parâmetros de Q-ball. Numa segunda parte, consideraremos a existência de objetos bosónicos na presença de efeitos gravitacionais. A existência de \bolhas" localizadas, aproximadamente estacionárias, do campo gravitacional e eletromagnético clássico - geons foi conjeturada há mais de meio século. Se se insistir em soluções estáticas, as configurações topologicamente triviais no eletro-vácuo são descartadas por teoremas de não-retorno para solitões. Mas os conceitos estacionários e assintoticamente planos de geons encontraram uma solução no vácuo escalar, onde podem existir \bolhas" de campo escalar localizados conhecidos como estrelas do bosões (escalares). Nesta tese, um método de Runge-Kutta de quarta ordem, com uma rotina de shooting, foi implementado para obter o diagrama de fase para obter uma estrela de bosões no estado fundamental, bem como uma unica solução para um estado excitado. Analisamos então o diagrama de fases obtido e algumas quantidades físicas obtidas a partir dele.
In the absence of gravitational e ects, the dispersiveness of the linear Klein-Gordon equation can be counter-balanced by introducing non-linear self-interactions of the scalar eld. When cancellation of non-linear and dispersive e ects occurs, selfreinforcing solitary wave packets emerge. If this solitary wave packets are formed by a single complex scalar eld, a Q-ball is formed. The most generic type of Qballs, known as gauged spinning Q-balls, possess a spinning phase and an electrical charge. In this thesis, after a brief introduction of the model and some physical and asymptotical properties of Q-ball solutions, a spectroscopic method to decompose the several Q-ball elds is introduced, and used to obtained, and analise the latter's. To perform the spectroscopic analises and compare between the possible Q-ball solutions, some physical quantities { namely the electrical charge, Noether charge, energy, gyromagnetic factor and magnetic dipole moment { are retrieved. In a second part, the existence of bosonic objects in the presence of gravitational e ects is going to be considered. The existence of localized, approximately stationary, lumps of the classical gravitational and electromagnetic eld { geons { was conjectured more than half a century ago. If one insists on exact stationarity, topologically trivial con gurations in electro-vacuum are ruled out by no-go theorems for solitons. But stationary, asymptotically at geons found a realization in scalar-vacuum, where everywhere non-singular, localized eld lumps exist, known as (scalar) boson stars. To numerically obtain the boson star solutions, a four order Runge-Kutta method with a shooting routine was implemented. With it, the phase parameter diagram for the fundamental state and single excited state, are obtained. We then analise the obtained phase diagram, study the di erent branches and some physical quantities
Almergren, Joachim. "Energy and Rotation in Relativistic Astrophysics". Doctoral thesis, SISSA, 2003. http://hdl.handle.net/20.500.11767/4245.
Texto completoMoe, Maxwell y Stefano Rosanne Di. "Mind Your Ps and Qs: The Interrelation between Period (P) and Mass-ratio (Q) Distributions of Binary Stars". IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/624451.
Texto completoSamadov, Hidayat. "Analyzing Reservoir Thermal Behavior By Using Thermal Simulation Model (sector Model In Stars)". Master's thesis, METU, 2011. http://etd.lib.metu.edu.tr/upload/12613336/index.pdf.
Texto completohowever no significant changes were observed due to iteration number differences and refined grids. These latter cases showed clearly that variations of temperature don&rsquo
t occur only due to geothermal gradient, but also pressure and saturation changes. On the whole, BHT can be used to get data ranging from daily gas-oil ratios to interwell connection if analyzed correctly.
Joseph, Craig L. "Q-nucleosynthesis : implications for stellar evolution /". The Ohio State University, 1985. http://rave.ohiolink.edu/etdc/view?acc_num=osu1487260531956577.
Texto completoMurphy, Simon James. "Investigating the A-type stars using Kepler data". Thesis, University of Central Lancashire, 2013. http://clok.uclan.ac.uk/9635/.
Texto completoBrookes, Diane Patricia. "Interferometric radio observations of the interactive winds of massive stars". Thesis, University of Birmingham, 2016. http://etheses.bham.ac.uk//id/eprint/6749/.
Texto completoClaas, Ralf Frederik [Verfasser], zu Heringdorf Dagmar [Akademischer Betreuer] Meyer y Holger [Akademischer Betreuer] Stark. "Regulation der Sphingosinkinase-1 durch G alpha q / Ralf Frederik Claas. Gutachter: Holger Stark ; Dagmar Meyer zu Heringdorf. Betreuer: Dagmar Meyer zu Heringdorf". Frankfurt am Main : Univ.-Bibliothek Frankfurt am Main, 2012. http://d-nb.info/1044093684/34.
Texto completoMüller, Stefanie. "Improving the Usability of a Q&A Platform : A design process based on the principles of Lean UX – adapted to a given start-up environment". Thesis, Tekniska Högskolan, Högskolan i Jönköping, JTH, Datateknik och informatik, 2019. http://urn.kb.se/resolve?urn=urn:nbn:se:hj:diva-45309.
Texto completoFelicetti, Roberto. "Field Current Control for the Damping of Rotor Oscillations and for the Alternative Start of Synchronous Machines : Further Innovative Applications of Field Current Active Control besides UMP-Compensation". Thesis, Uppsala universitet, Institutionen för teknikvetenskaper, 2018. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-353669.
Texto completoLibros sobre el tema "Q-stars"
Luke, Crampton, ed. Q encyclopedia of rock stars. London: Dorling Kindersley, 1996.
Buscar texto completoInc, Game Counselor. Game Counselor's Answer Book for Nintendo Players. Redmond, USA: Microsoft Pr, 1991.
Buscar texto completoInc, Game Counsellor, ed. The Game Counsellor's answer book for Nintendo Game players: Hundredsof questions -and answers - about more than 250 popular Nintendo Games. Redmond, Washington: Microsoft Press, 1991.
Buscar texto completoAwesome Super Nintendo Secrets 2. Lahaina, USA: Sandwich Islands Publishing, 1993.
Buscar texto completoCrampton, Luke y Daffyd Rees. Q Rock Stars Encyclopedia. Edition Olms, 1999.
Buscar texto completoThomson, Sarah L. Extreme Stars! Q&A (Smithsonian Q & A (Children's Paperback)). Collins, 2006.
Buscar texto completoThomson, Sarah L. Extreme Stars! Q&A (Smithsonian Q & A (Children's Paperback)). Collins, 2006.
Buscar texto completoExtreme Stars! Q&A (Smithsonian Q & A (Children's Cloth)). Collins, 2006.
Buscar texto completoThomson, Sarah L. Extreme Stars! Q&A (Smithsonian Q & A (Children's Cloth)). Collins, 2006.
Buscar texto completoTracer, Grey. Q Stars and Neighbors: Meet Ace and K. Independently Published, 2017.
Buscar texto completoCapítulos de libros sobre el tema "Q-stars"
Lynn, B. W. "Q-Stars". En Phase Structure of Strongly Interacting Matter, 204–15. Berlin, Heidelberg: Springer Berlin Heidelberg, 1990. http://dx.doi.org/10.1007/978-3-642-87821-3_7.
Texto completoAidelman, Yael, Carlos Escudero, Franco Ronchetti, Facundo Quiroga y Laura Lanzarini. "Reddening-Free Q Indices to Identify Be Star Candidates". En Communications in Computer and Information Science, 111–23. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-61218-4_8.
Texto completoDeutsch, Nurit Novis y Maria Klingenberg. "Who Relates to the Divine as Feminine? Transnational Consensus and Outliers Among Young Adults". En The Diversity Of Worldviews Among Young Adults, 133–51. Cham: Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-030-94691-3_7.
Texto completo"Q". En Shooting Stars of the Small Screen, 269–70. University of Texas Press, 2009. http://dx.doi.org/10.7560/718494-020.
Texto completoFahlstedt, Kim Khavar. "Charlie Chan’s Last Mystery, or the Transcultural Disappearance of Warner Oland". En Nordic Film Cultures and Cinemas of Elsewhere, 42–52. Edinburgh University Press, 2019. http://dx.doi.org/10.3366/edinburgh/9781474438056.003.0003.
Texto completoChuang, Ching-Ho. "Allmächtig oder hochmütig? Q in Star Trek". En Superbia – Hochmut und Stolz in Kultur und Literatur, 183–212. Psychosozial-Verlag, 2014. http://dx.doi.org/10.30820/9783837969047-183.
Texto completo"q-Analogs of Multiple Harmonic (Star) Sums". En Series on Number Theory and Its Applications, 279–304. WORLD SCIENTIFIC, 2016. http://dx.doi.org/10.1142/9789814689403_0009.
Texto completo"q-Analogs of Multiple Zeta (Star) Values". En Series on Number Theory and Its Applications, 365–417. WORLD SCIENTIFIC, 2016. http://dx.doi.org/10.1142/9789814689403_0012.
Texto completoBriscoe, J. "The Language and Style of the Fragmentary Republican Historians". En Aspects of the Language of Latin Prose. British Academy, 2005. http://dx.doi.org/10.5871/bacad/9780197263327.003.0003.
Texto completoDyer, Dr Karen. "1. Exam Skills for Success in Tort Law". En Concentrate Questions and Answers Tort Law, 1–4. Oxford University Press, 2019. http://dx.doi.org/10.1093/he/9780198745297.003.0001.
Texto completoActas de conferencias sobre el tema "Q-stars"
Verbin, Y., Arttu Rajantie, Carlo Contaldi, Paul Dauncey y Horace Stoica. "Sigma Model Q-balls and Q-Stars". En PARTICLES, STRINGS, AND COSMOLOGY. AIP, 2007. http://dx.doi.org/10.1063/1.2823779.
Texto completoVERBIN, Y. "SOLITONIC AND NON-SOLITONIC Q-STARS". En Proceedings of the MG11 Meeting on General Relativity. World Scientific Publishing Company, 2008. http://dx.doi.org/10.1142/9789812834300_0396.
Texto completoSeleznev, A. F. y A. A. Malofeeva. "A search of unresolved binaries in open clusters by the photometry data in visible and infrared". En 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/vak2021.2022.1.1.194.
Texto completoMustonen, M. T., J. Suhonen, Livius Trache, Alexei Smirnov y Sabin Stoica. "Beyond low beta-decay Q values". En EXOTIC NUCLEI AND NUCLEAR∕PARTICLE ASTROPHYSICS (III): From Nuclei to Stars. AIP, 2010. http://dx.doi.org/10.1063/1.3527233.
Texto completoBock, J., N. Bangemann y S. Paepke. "Which breast scar is the breast-Q star?" En 41. Jahrestagung der Deutschen Gesellschaft für Senologie e.V. – Gemeinsam gegen Brustkrebs: optimale Behandlung für jede Patientin. Georg Thieme Verlag, 2022. http://dx.doi.org/10.1055/s-0042-1748350.
Texto completoFrey, Robert y Bruno Thedrez. "Interpretation of Intracavity Instabilities in Terms of Dynamic Stark Effect". En Optical Bistability. Washington, D.C.: Optica Publishing Group, 1988. http://dx.doi.org/10.1364/obi.1988.we.7.
Texto completoXiong, Wei y Ana V. Stankovic. "Program start fluorescent ballast with clamped-Q resonant filament heating circuit". En 2014 IEEE Industry Applications Society Annual Meeting. IEEE, 2014. http://dx.doi.org/10.1109/ias.2014.6978433.
Texto completoCherepashchuk, A. M., T. S. Khruzina y A. I. Bogomazov. "Parameters of Sco X-1". En 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.
Texto completoAndriollo, M., G. Bettanini, G. Martinelli, A. Morini y A. Tortella. "Analysis of Double Star Permanent Magnet Synchronous Generators by a General Decoupled d-q Model". En 2007 IEEE International Electric Machines & Drives Conference. IEEE, 2007. http://dx.doi.org/10.1109/iemdc.2007.383544.
Texto completoBuyalo, M. S., I. M. Gadzhiyev, N. D. Il'inskaya, A. A. Usikova, V. N. Nevedomskiy, A. Yu Egorov y E. L. Portnoi. "Mode-locking and Q-switching in 1.06 μm two-sectional QW lasers due to stark effect". En 2016 International Conference Laser Optics (LO). IEEE, 2016. http://dx.doi.org/10.1109/lo.2016.7549717.
Texto completoInformes sobre el tema "Q-stars"
Hochron, D. R., B. W. Lynn y S. B. Selipsky. An upper bound on Q-star masses. Office of Scientific and Technical Information (OSTI), junio de 1992. http://dx.doi.org/10.2172/94554.
Texto completoFarahbod, A. M. y J. F. Cassidy. An overview of seismic attenuation in the Eastern Canadian Arctic and the Hudson Bay Complex, Manitoba, Newfoundland and Labrador, Nunavut, Ontario, and Quebec. Natural Resources Canada/CMSS/Information Management, 2022. http://dx.doi.org/10.4095/330396.
Texto completoFarahbod, A. M. y J. F. Cassidy. An overview of seismic attenuation in the Northern Appalachians Seismic Zone, New Brunswick and Nova Scotia. Natural Resources Canada/CMSS/Information Management, 2022. http://dx.doi.org/10.4095/329702.
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