Bibliografías temáticas / Cosmological phase transitions

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Literatura académica sobre el tema "Cosmological phase transitions"

Autor: Grafiati
Publicado: 30 de noviembre de 2024
Última modificación: 31 de julio de 2025

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Artículos de revistas sobre el tema "Cosmological phase transitions"

1

KIM, SANG PYO. "DYNAMICAL THEORY OF PHASE TRANSITIONS AND COSMOLOGICAL EW AND QCD PHASE TRANSITIONS." Modern Physics Letters A 23, no. 17n20 (2008): 1325–35. http://dx.doi.org/10.1142/s0217732308027692.

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We critically review the cosmological EW and QCD phase transitions. The EW and QCD phase transitions would have proceeded dynamically since the expansion of the universe determines the quench rate and critical behaviors at the onset of phase transition slow down the phase transition. We introduce a real-time quench model for dynamical phase transitions and describe the evolution using a canonical real-time formalism. We find the correlation function, the correlation length and time and then discuss the cosmological implications of dynamical phase transitions on EW and QCD phase transitions in
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2

Athron, Peter, Csaba Balázs, and Lachlan Morris. "Supercool subtleties of cosmological phase transitions." Journal of Cosmology and Astroparticle Physics 2023, no. 03 (2023): 006. http://dx.doi.org/10.1088/1475-7516/2023/03/006.

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Abstract We investigate rarely explored details of supercooled cosmological first-order phase transitions at the electroweak scale, which may lead to strong gravitational wave signals or explain the cosmic baryon asymmetry. The nucleation temperature is often used in phase transition analyses, and is defined through the nucleation condition: on average one bubble has nucleated per Hubble volume. We argue that the nucleation temperature is neither a fundamental nor essential quantity in phase transition analysis. We illustrate scenarios where a transition can complete without satisfying the nuc
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3

Buckley, Matthew R., Peizhi Du, Nicolas Fernandez, and Mitchell J. Weikert. "Dark radiation isocurvature from cosmological phase transitions." Journal of Cosmology and Astroparticle Physics 2024, no. 07 (2024): 031. http://dx.doi.org/10.1088/1475-7516/2024/07/031.

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Abstract Cosmological first order phase transitions are typically associated with physics beyond the Standard Model, and thus of great theoretical and observational interest. Models of phase transitions where the energy is mostly converted to dark radiation can be constrained through limits on the dark radiation energy density (parameterized by ΔN eff). However, the current constraint (ΔN eff < 0.3) assumes the perturbations are adiabatic. We point out that a broad class of non-thermal first order phase transitions that start during inflation but do not complete until after reheating leave
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4

Hogan, C. J. "Gravitational radiation from cosmological phase transitions." Monthly Notices of the Royal Astronomical Society 218, no. 4 (1986): 629–36. http://dx.doi.org/10.1093/mnras/218.4.629.

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MÉGEVAND, ARIEL. "GRAVITATIONAL WAVES FROM COSMOLOGICAL PHASE TRANSITIONS." International Journal of Modern Physics A 24, no. 08n09 (2009): 1541–44. http://dx.doi.org/10.1142/s0217751x09044966.

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6

Kurki-Suonio, H., and M. Laine. "Supersonic deflagrations in cosmological phase transitions." Physical Review D 51, no. 10 (1995): 5431–37. http://dx.doi.org/10.1103/physrevd.51.5431.

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Vachaspati, Tanmay. "Magnetic fields from cosmological phase transitions." Physics Letters B 265, no. 3-4 (1991): 258–61. http://dx.doi.org/10.1016/0370-2693(91)90051-q.

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Durrer, Ruth. "Gravitational waves from cosmological phase transitions." Journal of Physics: Conference Series 222 (April 1, 2010): 012021. http://dx.doi.org/10.1088/1742-6596/222/1/012021.

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Athron, Peter, Lachlan Morris, and Zhongxiu Xu. "How robust are gravitational wave predictions from cosmological phase transitions?" Journal of Cosmology and Astroparticle Physics 2024, no. 05 (2024): 075. http://dx.doi.org/10.1088/1475-7516/2024/05/075.

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Abstract Gravitational wave (GW) predictions of cosmological phase transitions are almost invariably evaluated at either the nucleation or percolation temperature. We investigate the effect of the transition temperature choice on GW predictions, for phase transitions with weak, intermediate and strong supercooling. We find that the peak amplitude of the GW signal varies by a factor of a few for weakly supercooled phase transitions, and by an order of magnitude for strongly supercooled phase transitions. The variation in amplitude for even weakly supercooled phase transitions can be several ord
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10

Jinno, Ryusuke, Thomas Konstandin, Henrique Rubira, and Isak Stomberg. "Higgsless simulations of cosmological phase transitions and gravitational waves." Journal of Cosmology and Astroparticle Physics 2023, no. 02 (2023): 011. http://dx.doi.org/10.1088/1475-7516/2023/02/011.

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Abstract First-order cosmological phase transitions in the early Universe source sound waves and, subsequently, a background of stochastic gravitational waves. Currently, predictions of these gravitational waves rely heavily on simulations of a Higgs field coupled to the plasma of the early Universe, the former providing the latent heat of the phase transition. Numerically, this is a rather demanding task since several length scales enter the dynamics. From smallest to largest, these are the thickness of the Higgs interface separating the different phases, the shell thickness of the sound wave
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Tesis sobre el tema "Cosmological phase transitions"

1

Ferreira, Pedro Tonnies Gil. "Observational consequences of cosmological phase transitions." Thesis, Imperial College London, 1995. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.338692.

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Larsson, Sebastian E. "Topological defects from cosmological phase transitions." Thesis, University of Oxford, 1998. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.298309.

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Adams, Jennifer Anne. "Cosmological phase transitions : techniques and phenomenology." Thesis, University of Oxford, 1995. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.306935.

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Lilley, Matthew James. "Cosmological phase transitions and primordial magnetic fields." Thesis, University of Cambridge, 2001. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.621001.

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5

Faure, Rémi. "Neutrinos, cosmological phase transitions and the matter-antimatter asymmetry of the Universe." Electronic Thesis or Diss., université Paris-Saclay, 2024. http://www.theses.fr/2024UPASP081.

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L'asymétrie entre matière et antimatière est un problème non résolu de la cosmologie. Une approche populaire pour l'expliquer est la leptogénèse avec des neutrinos stériles, qui sont des particules motivées expérimentalement pour expliquer les masses des neutrinos actifs du Modèle Standard. Il est possible d'inclure dans les scénarios de leptogénèse une transition de phase cosmologique qui donne leur masse aux neutrinos stériles. Cette idée est intéressante phénoménologiquement, car une transition de phase produit des ondes gravitationnelles pouvant être détectées. À la température de la trans
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6

Dichtl, Maximilian. "Aspects of cosmological first order phase transitions : propagation of ultra-relativistic shells, heavy dark matter, and baryogenesis." Electronic Thesis or Diss., Sorbonne université, 2024. http://www.theses.fr/2024SORUS181.

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Les transitions de phase du premier ordre (PT) dans l'univers primitif se produisent par la nucléation de bulles dont les parois peuvent se dilater à des vitesses ultra-relativistes. Les interactions du bain thermique à la paroi produisent des particules qui s'accumulent dans des coquilles à la paroi. Les coquilles évoluent jusqu'à ce qu'elles entrent en collision avec celles des bulles voisines. Dans cette thèse, nous étudions d'abord l'évolution de ces coquilles, en incluant pour la première fois les interactions de changement de nombre de la coquille à l'intérieur d'elle-même et avec le bai
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7

Martin, Adrian Peter. "Cosmological phase transition phenomena." Thesis, University of Cambridge, 1995. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.389880.

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8

Chowdhury, Talal Ahmed. "A Possible Link between the Electroweak Phase Transition and the Dark Matter of the Universe." Doctoral thesis, SISSA, 2014. http://hdl.handle.net/20.500.11767/3883.

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A possible connection between the dark matter and strong first order electroweak phase transition, which is an essential ingredient of the electroweak baryogenesis, has been explored in this thesis. It is shown that the extension of the Standard Model's minimal Higgs sector with an inert $SU(2)_L$ scalar doublet can provide light dark matter candidate and simultaneously induce a strong first order phase transition. There is however no symmetry reason to prevent the extension using scalars with higher $SU(2)_L$ representations. Therefore, by making random scans over the models' paramete
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9

Manning, Adrian Gordon. "Quantum Fields in Curved Spacetime with Cosmological and Gravitational Wave Implications." Thesis, The University of Sydney, 2018. http://hdl.handle.net/2123/17804.

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A range of novel ideas, covering both general relativity and quantum field theory are introduced and explored. An analytic procedure for theories that modify the stress-energy-tensor in general relativity is examined which compares predicted deviations in the gravitational wave radiation from binary black hole mergers to the observed waveform from recent detections, i.e GW150914. This is applied directly to the theory of non-commutative spacetimes, which ultimately constrains the scale of non-commutative spacetime up to the Planck scale, some 15 orders of magnitude improvement on previous boun
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10

Scott, Pat. "Searches for Particle Dark Matter Dark stars, dark galaxies, dark halos and global supersymmetric fits /." Doctoral thesis, Stockholm : Department of Physics, Stockholm University, 2010. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-38221.

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Diss. (sammanfattning) Stockholm : Stockholms universitet, 2010.<br>At the time of the doctoral defense, the following papers were unpublished and had a status as follows: Paper 5: Accepted. Paper 6: Submitted. Härtill 6 uppsatser.
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Libros sobre el tema "Cosmological phase transitions"

1

Nagasawa, Michiyasu. Cosmological phase transitions and evolution of topological defects. University of Tokyo, 1993.

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2

National Aeronautics and Space Administration (NASA) Staff. Late Time Cosmological Phase Transitions 1: Particle Physics Models and Cosmic Evolution. Independently Published, 2018.

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3

Maggiore, Michele. Stochastic backgrounds of cosmological origin. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198570899.003.0013.

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Characteristic frequency of relic GWs. Production mechanisms of GWs in the early universe: preheating, phase transitions, cosmic strings, alternatives to inflation. Bounds on primordial GW backgrounds: nucleosynthesis bound, bounds from CMB, observational limits at interferometers.
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4

Maggiore, Michele. Gravitational Waves. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198570899.001.0001.

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A comprehensive and detailed account of the physics of gravitational waves and their role in astrophysics and cosmology. The part on astrophysical sources of gravitational waves includes chapters on GWs from supernovae, neutron stars (neutron star normal modes, CFS instability, r-modes), black-hole perturbation theory (Regge-Wheeler and Zerilli equations, Teukoslky equation for rotating BHs, quasi-normal modes) coalescing compact binaries (effective one-body formalism, numerical relativity), discovery of gravitational waves at the advanced LIGO interferometers (discoveries of GW150914, GW15122
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5

Late time cosmological phase transition I: Particle physics models and cosmic evolution. Fermi National Accelerator Laboratory, 1991.

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Capítulos de libros sobre el tema "Cosmological phase transitions"

1

Kolb, Edward W. "Cosmological Phase Transitions." In Gravitation in Astrophysics. Springer US, 1987. http://dx.doi.org/10.1007/978-1-4613-1897-2_11.

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2

Schramm, David N. "Late-Time Cosmological Phase Transitions." In Primordial Nucleosynthesis and Evolution of Early Universe. Springer Netherlands, 1991. http://dx.doi.org/10.1007/978-94-011-3410-1_31.

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3

Boyanovsky, D., H. J. Vega, and M. Simionato. "Primordial magnetic fields from cosmological phase transitions." In The Early Universe and the Cosmic Microwave Background: Theory and Observations. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-007-1058-0_5.

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4

Bäuerle, C., Yu M. Bunkov, S. N. Fisher, and H. Godfrin. "The ‘Grenoble’ Cosmological Experiment." In Topological Defects and the Non-Equilibrium Dynamics of Symmetry Breaking Phase Transitions. Springer Netherlands, 2000. http://dx.doi.org/10.1007/978-94-011-4106-2_6.

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5

Khlopov, Maxim Yu, and Sergei G. Rubin. "High Density Regions from First-Order Phase Transitions." In Cosmological Pattern of Microphysics in the Inflationary Universe. Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-1-4020-2650-8_8.

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6

Goldenfeld, Nigel. "Dynamics of Cosmological phase transitions: What can we learn from condensed matter physics?" In Formation and Interactions of Topological Defects. Springer US, 1995. http://dx.doi.org/10.1007/978-1-4615-1883-9_4.

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7

Bunkov, Yu M. "“Aurore De Venise” — Cosmological Scenario of the A-B Phase Transition in Superfluid 3He." In Topological Defects and the Non-Equilibrium Dynamics of Symmetry Breaking Phase Transitions. Springer Netherlands, 2000. http://dx.doi.org/10.1007/978-94-011-4106-2_7.

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8

Gouttenoire, Yann. "First-Order Cosmological Phase Transition." In Beyond the Standard Model Cocktail. Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-031-11862-3_6.

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Becker, Jörg D., and Lutz Castell. "Ur Theory and Cosmological Phase Transition." In Time, Quantum and Information. Springer Berlin Heidelberg, 2003. http://dx.doi.org/10.1007/978-3-662-10557-3_29.

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Stock, Reinhard. "Relativistic Nucleus-Nucleus Collisions and the QCD Matter Phase Diagram." In Particle Physics Reference Library. Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-38207-0_7.

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AbstractThis review will be concerned with our knowledge of extended matter under the governance of strong interaction, in short: QCD matter. Strictly speaking, the hadrons are representing the first layer of extended QCD architecture. In fact we encounter the characteristic phenomena of confinement as distances grow to the scale of 1 fm (i.e. hadron size): loss of the chiral symmetry property of the elementary QCD Lagrangian via non-perturbative generation of “massive” quark and gluon condensates, that replace the bare QCD vacuum. However, given such first experiences of transition from short
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Actas de conferencias sobre el tema "Cosmological phase transitions"

1

Matteini, Marco. "Analytical Euclidean action for cosmological phase transitions." In 2nd Training School and General Meeting of the COST Action COSMIC WISPers (CA21106). Sissa Medialab, 2025. https://doi.org/10.22323/1.474.0065.

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Quirós, Mariano. "Cosmological phase transitions and baryogenesis." In The sixth Mexican workshop on particles and fields. American Institute of Physics, 1998. http://dx.doi.org/10.1063/1.56628.

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3

Rummukainen, Kari, Stephan J. Huber, Mark B. Hindmarsh, and David Weir. "Gravitational waves from cosmological first order phase transitions." In The 33rd International Symposium on Lattice Field Theory. Sissa Medialab, 2016. http://dx.doi.org/10.22323/1.251.0233.

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4

Boyanovsky, D. "Primordial Magnetic Fields from Out of Equilibrium Cosmological Phase Transitions." In MAGNETIC FIELDS IN THE UNIVERSE: From Laboratory and Stars to Primordial Structures. AIP, 2005. http://dx.doi.org/10.1063/1.2077205.

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5

Rakic, Aleksandar, Dennis Simon, Julian Adamek, and Jens Niemeyer. "Cosmological first-order phase transitions beyond the standard inflationary scenario." In International Workshop on Cosmic Structure and Evolution. Sissa Medialab, 2010. http://dx.doi.org/10.22323/1.097.0007.

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Dumin, Yu V. "ON THE INFLUENCE OF EINSTEIN–PODOLSKY–ROSEN EFFECT ON THE DOMAIN WALL FORMATION DURING THE COSMOLOGICAL PHASE TRANSITIONS." In Proceedings of the Tenth Lomonosov Conference on Elementary Particle Physics. WORLD SCIENTIFIC, 2003. http://dx.doi.org/10.1142/9789812704948_0037.

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Romero-Rodríguez, Alba. "Implications for first-order cosmological phase transitions and the formation of primordial black holes from the third LIGO-Virgo observing run." In The European Physical Society Conference on High Energy Physics. Sissa Medialab, 2022. http://dx.doi.org/10.22323/1.398.0113.

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HWANG, W. Y. P. "SOME THOUGHTS ON THE COSMOLOGICAL QCD PHASE TRANSITION." In Statistical Physics, High Energy, Condensed Matter and Mathematical Physics - The Conference in Honor of C. N. Yang'S 85th Birthday. WORLD SCIENTIFIC, 2008. http://dx.doi.org/10.1142/9789812794185_0005.

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Sinha, Bikash. "Relics of the Cosmological Quark-Hadron Phase Transition." In Proceedings of the Sixth International Workshop. WORLD SCIENTIFIC, 2001. http://dx.doi.org/10.1142/9789812799814_0007.

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Tawfik, A., and Shaaban Khalil. "Cosmological Consequences of QCD Phase Transition(s) in Early Universe." In THE DARK SIDE OF THE UNIVERSE: 4th International Workshop on the Dark Side of the Universe. AIP, 2009. http://dx.doi.org/10.1063/1.3131505.

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Informes sobre el tema "Cosmological phase transitions"

1

Kolb, E. W. Cosmological phase transitions. Office of Scientific and Technical Information (OSTI), 1986. http://dx.doi.org/10.2172/5086987.

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Lindesay, James V., and H. Pierre Noyes. Evidence for a Cosmological Phase Transition on the TeVScale. Office of Scientific and Technical Information (OSTI), 2005. http://dx.doi.org/10.2172/878749.

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