Interstellar travel guide: Chronicles of a violent universe

Autors/ores

  • Manel Perucho University of Valencia (Spain).
  • José A. Font University of Valencia (Spain).

DOI:

https://doi.org/10.7203/metode.7.8821

Paraules clau:

relativity, black holes, neutron stars, active galaxies, hydrodynamics

Resum

In contrast to observations from our local viewpoint, the universe is extremely violent. Explosions of massive stars, X-ray and gamma-ray binary stars, and active galaxies are related to the presence of compact objects such as neutron stars or black holes. Processes such as matter accretion or the formation and release of relativistic plasma jets are responsible for the generation of large amounts of high-energy radiation, caused by the acceleration of elementary particles, and have a significant impact in their surroundings. Moreover, they are related to the generation of gravitational waves: vibrations in spacetime produced by the acceleration of compact massive objects that produce strong curvatures. These systems are studied within the framework of the general and special relativity theories. In this article, we summarise several of the most well-known astrophysical scenarios, and offer a brief description of what we currently know about them.

 

Descàrregues

Les dades de descàrrega encara no estan disponibles.

Biografies de l'autor/a

Manel Perucho, University of Valencia (Spain).

Tenured professor of Physics at the University of Valencia (Spain). His research focuses on the study of relativistic fluids in different astrophysical scenarios using relativistic hydrodynamics and magnetohydrodynamics numerical simulations. Among the scenarios he studies, are the jets generated in active galactic nuclei or in binary X-ray or gamma-ray stars. He was the principal investigator on different supercomputer calculation projects as well as on an international observation project with the Russian space telescope Radioastron.

José A. Font, University of Valencia (Spain).

Tenured professor of Physics at the University of Valencia (Spain). His field of research is relativistic astrophysics and in particular, he studies neutron stars, black holes, and gravitational radiation using computational tools such as relativistic hydrodynamics or magnetohydrodynamics and numerical relativity. He was the president of the Spanish Society of Gravitation and Relativity and now coordinates the Valencia group for the Virgo collaboration and directs the Department of Astronomy and Astrophysics in the University of Valencia.

Referències

Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M. R., Acernese, F., Ackley, K., … Zweizig, J. (2016). Observation of gravitational waves from a binary black hole merger. Physical Review Letters, 116(6), 061102. doi: 10.1103/PhysRevLett.116.061102

Blandford, R. D., & Payne, D. G. (1982). Hydromagnetic flows from accretion discs and the production of radio jets. Monthly Notices of the Royal Astronomical Society, 199(4), 883–903. doi: 10.1093/mnras/199.4.883

Blandford, R. D., & Znajek, R. L. (1977). Electromagnetic extraction of energy from Kerr black holes. Monthly Notices of the Royal Astronomical Society, 179(3), 433–456. doi: 10.1093/mnras/179.3.433

Bolton, C. T. (1972). Identification of Cygnus X-1 with HDE 226868. Nature, 235, 271–273. doi: 10.1038/235271b0

Font, J. A., Sintes, A. M., & Sopuerta, C. F. (2015). Gravitational waves with the SKA. In M. A. Pérez-Torres (Ed.), The Spanish Square Kilometer Array white book (pp. 29–36). Barcelona: Sociedad Española de Astronomía. Retrieved from https://arxiv.org/abs/1506.03474

Gehrels, N., Ramírez-Ruiz, E., & Fox., D. B. (2009). Gamma-ray bursts in the Swift era. Annual Review of Astronomy and Astrophysics, 47, 567–617. doi: 10.1146/annurev.astro.46.060407.145147

Genzel, R., Eisenhauer, F., & Gillessen, S. (2010). The Galactic Center massive black hole and nuclear star cluster. Reviews of Modern Physics, 82, 3121–1395. doi: 10.1103/RevModPhys.82.3121

Goddi, C., Falcke, H., Kramer, M., Rezzolla, L., Brinkerink, T., Bronzwaer, T., ... Zhidenko, A. (2016). BlackHoleCam: fundamental physics of the galactic center. International Journal of Modern Physics D, 1730001. doi: 10.1142/S0218271817300014

Hewish, A., Bell, S. J., Pilkington, J. D. H., Scott, P. F., & Collins, R. A. (1968). Observation of a rapidly pulsating radio source. Nature, 217, 709–713. doi: 10.1038/217709a0

Hulse, R. A., & Taylor, J. H. (1975). Discovery of a pulsar in a binary system. Astrophysical Journal, 195, L51–L53. doi: 10.1086/181708

Janka, H. T. (2012). Explosion mechanisms of core-collapse supernovae. Annual Review of Nuclear and Particle Science, 62, 407–451. doi: 10.1146/annurev-nucl-102711-094901

Mościbrodzka, M., Falcke, H., Shiokawa, H., & Gammie, C. F. (2014). Observational appearance of inefficient accretion flows and jets in 3D GRMHD simulations: Application to Sagittarius A*. Astronomy & Astrophysics, 570, A7. doi: 10.1051/0004-6361/201424358

Netzer, H. (2013). The physics and evolution of active galactic nuclei. Cambridge: Cambridge University Press.

Piran, T., & Jiménez, R. (2014). Possible role of gamma ray bursts on life extinction in the universe. Physical Review Letters, 113(23), 231102. doi: 10.1103/PhysRevLett.113.231102

Shapiro, S. L., & Teukolsky, S. A. (2007). Black holes, white dwarfs, and neutron stars: The physics of compact objects. New York: Wiley Online Library. (Original work published in 1983). doi: 10.1002/9783527617661

Webster, B. L., & Murdin, P. (1972). Cygnus X-1 —A spectroscopic binary with a heavy companion? Nature, 235, 37–38. doi: 10.1038/235037a0

Descàrregues

Publicades

2017-06-20

Com citar

Perucho, M., & Font, J. A. (2017). Interstellar travel guide: Chronicles of a violent universe. Metode Science Studies Jornal, (7), 143–151. https://doi.org/10.7203/metode.7.8821
Metrics
Views/Downloads
  • Resum
    1485
  • PDF
    335

Número

Unravelling science: Pulling the thread of knowledge (2017)

Secció

L'univers violent. Astrofísica d'altes energies i cosmologia del segle XXI

Llicència

Tots els documents inclosos en OJS són d'accés lliure i propietat dels seus autors.

Els autors que publiquen en aquesta revista estan d'acord amb els següents termes:

    1. Els autors conserven els drets d'autor i garanteixen a la revista el dret a la primera publicació del treball, llicenciat baix una llicència de Reconeixement-NoComercial-SenseObraDerivada 4.0 Internacional de Creative Commons, que permet a altres compartir el treball amb un reconeixement de l'autoria del treball i citant la publicació inicial en aquesta revista.
    2. Es permet i s'anima els autors a difondre la versió definitiva dels seus treballs electrònicament a través de pàgines personals i institucionals (repositoris institucionals, pàgines web personals o perfils a xarxes professionals o acadèmiques) una vegada publicat el treball.

Metrics

Articles similars

<< < > >> 

També podeu iniciar una cerca avançada per similitud per a aquest article.