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Letteratura scientifica selezionata sul tema "Astrophysics"

Autore: Grafiati

Pubblicato: 4 giugno 2021

Ultima modifica: 30 novembre 2024

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Articoli di riviste sul tema "Astrophysics"

1

Depalo, Rosanna. "Nuclear Astrophysics Deep Underground". International Journal of Modern Physics: Conference Series 46 (gennaio 2018): 1860003. http://dx.doi.org/10.1142/s2010194518600030.

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Cross sections of nuclear reactions relevant for astrophysics are crucial ingredients to understand the energy generation inside stars and the synthesis of the elements. At astrophysical energies, nuclear cross sections are often too small to be measured in laboratories on the Earth surface, where the signal would be overwhelmed by the cosmic-ray induced background. LUNA is a unique Nuclear Astrophysics experiment located at Gran Sasso National Laboratories. The extremely low background achieved at LUNA allows to measure nuclear cross sections directly at the energies of astrophysical interest. Over the years, many crucial reactions involved in stellar hydrogen burning as well as Big Bang nucleosynthesis have been measured at LUNA. The present contribution provides an overview on underground Nuclear Astrophysics as well as the latest results and future perspectives of the LUNA experiment.

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2

OSTERBROCK, D. E. "An Astrophysical Concept: Accretion Power in Astrophysics." Science 233, n. 4763 (1 agosto 1986): 582–83. http://dx.doi.org/10.1126/science.233.4763.582.

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3

Longair, Malcolm, e Martin Rees. "Geoffrey Ronald Burbidge. 24 September 1925 — 26 January 2010". Biographical Memoirs of Fellows of the Royal Society 63 (gennaio 2017): 55–78. http://dx.doi.org/10.1098/rsbm.2017.0002.

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Geoffrey (Geoff) Burbidge's career spanned the tumultuous years when astronomy was transformed from a purely optical science to a multi-wavelength discipline through the development of new types of astronomy—radio, X-ray, γ -ray, cosmic ray physics. These offered new astrophysical and cosmological challenges, which he grasped with relish. To all of these disciplines, Geoff, often in collaboration with his wife Margaret Burbidge (FRS 1964), made pioneering contributions, particularly in the areas of the synthesis of the chemical elements, the physics of extragalactic radio sources, the rotation curves of galaxies, the dark matter problem in clusters of galaxies, the physics of accretion discs and the origin of cosmic rays. He also espoused less popular causes such as the non-cosmological nature of the redshifts of quasars and was sceptical about the standard Big Bang picture of the origin of the large-scale structure and dynamics of the Universe. He was a flamboyant and outspoken astrophysicist who challenged his colleagues about their deeply held views on all aspects of astrophysics and cosmology. His service to the community included five years as director of the US Kitt Peak National Observatory, based in Tucson, Arizona, and as a most effective editor of Annual Review of Astronomy and Astrophysics for over 30 years and the Astrophysical Journal.

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Gyürky, György. "Challenges and Requirements in High-Precision Nuclear Astrophysics Experiments". Universe 8, n. 4 (28 marzo 2022): 216. http://dx.doi.org/10.3390/universe8040216.

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In the 21th century astronomical observations, as well as astrophysical models, have become impressively precise. For a better understanding of the processes in stellar interiors, the nuclear physics of astrophysical relevance—known as nuclear astrophysics—must aim for similar precision, as such precision is not reached yet in many cases. This concerns both nuclear theory and experiment. In this paper, nuclear astrophysics experiments are put in focus. Through the example of various parameters playing a role in nuclear reaction studies, the difficulties of reaching high precision and the possible solutions are discussed.

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5

Adsley, Philip. "Transfer Reactions in Nuclear Astrophysics". EPJ Web of Conferences 275 (2023): 01001. http://dx.doi.org/10.1051/epjconf/202327501001.

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Transfer reactions are important tool in nuclear astrophysics. These reactions allow us to identify states in nuclei and to find the corresponding energies, to determine if these states can contribute to astrophysical nuclear reactions and ultimately to determine the strength of that contribution. In this paper,the basic details of how transfer reactions may be used in nuclear astrophysics are set out along with some common pitfalls to avoid.

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6

Descouvemont, P. "Astrophysica for Windows: a PC software for nuclear astrophysics". Nuclear Physics A 688, n. 1-2 (maggio 2001): 557–59. http://dx.doi.org/10.1016/s0375-9474(01)00786-2.

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7

EARDLEY, D. M. "Astrophysics: Relativistic Astrophysics." Science 232, n. 4751 (9 maggio 1986): 778. http://dx.doi.org/10.1126/science.232.4751.778-a.

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8

Lépine-Szily, Alinka, e Pierre Descouvemont. "Nuclear astrophysics: nucleosynthesis in the Universe". International Journal of Astrobiology 11, n. 4 (9 maggio 2012): 243–50. http://dx.doi.org/10.1017/s1473550412000158.

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AbstractNuclear astrophysics is a relatively young science; it is about half a century old. It is a multidisciplinary subject, since it combines nuclear physics with astrophysics and observations in astronomy. It also addresses fundamental issues in astrobiology through the formation of elements, in particular those required for a carbon-based life. In this paper, a rapid overview of nucleosynthesis is given, mainly from the point of view of nuclear physics. A short historical introduction is followed by the definition of the relevant nuclear parameters, such as nuclear reaction cross sections, astrophysical S-factors, the energy range defined by the Gamow peak and reaction rates. The different astrophysical scenarios that are the sites of nucleosynthesis, and different processes, cycles and chains that are responsible for the building of complex nuclei from the elementary hydrogen nuclei are then briefly described.

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9

Bingham, R., D. C. Speirs, B. J. Kellett, I. Vorgul, S. L. McConville, R. A. Cairns, A. W. Cross, A. D. R. Phelps e K. Ronald. "Laboratory astrophysics: Investigation of planetary and astrophysical maser emission". Space Science Reviews 178, n. 2-4 (8 marzo 2013): 695–713. http://dx.doi.org/10.1007/s11214-013-9963-z.

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10

Longair, Malcolm S. "Outside the Stars". International Astronomical Union Colloquium 137 (1993): 1–24. http://dx.doi.org/10.1017/s0252921100017395.

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It is a great pleasure and privilege to give the opening lecture at this IAU Colloquium “Inside the Stars”. It is particularly appropriate that it is held in Austria, the country of Ludwig Boltzmann whose name will appear explicitly or implicitly in every lecture.My task is to describe the astrophysical and cosmological setting within which our discussions will take place. I emphasise that I am an outsider at this colloquium in all possible senses. My own research interests are in the areas of high energy astrophysics, extragalactic research and astrophysical cosmology. In lecturing to my students, however, I emphasise that the subject of the present colloquium is at the very heart of virtually all astrophysics and these studies are quite essential in order to make sense of galaxies and extragalactic systems. If we did not have this confidence in our ability to understand the stars, at least in principle, we would worry about the reliability of the enormous astrophysical edifice which has been built up to explain the large scale features of our Universe. I also emphasise to my students that the study of the stars is among the most exact of the astrophysical sciences — in my enthusiastic moments, I claim that, in the very best of these studies, astrophysics approaches the precision of laboratory experiment. I hope to find many examples this week to reinforce this belief.From my perspective, what I need is a User’s Guide to Stars and Stellar Evolution, in other words, a reliable set of rules about the origin and evolution of stars in order to diagnose the physical properties of the systems I am trying to understand. I will illustrate the types of information we need by discussing three case studies in the areas of (i) high energy astrophysics, (ii) classical cosmology and (iii) astrophysical cosmology and the origin of galaxies. Necessarily, these studies will be far from complete, but I hope they will illustrate some of the issues which come up in these disciplines. In the course of the discussion, it will become apparent that I will touch upon essentially all branches of contemporary astrophysics. I will take very different approaches to the three case studies.

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Più fonti

Tesi sul tema "Astrophysics"

1

Baring, Matthew Geoffrey. "Pair plasmas in astrophysics". Thesis, University of Cambridge, 1988. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.279144.

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2

Price, Daniel James. "Magnetic fields in astrophysics". Thesis, University of Cambridge, 2004. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.616258.

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3

Reid, Giles Adrian. "Neutrino Oscillations in Astrophysics". Thesis, University of Canterbury. Physics and Astronomy, 2010. http://hdl.handle.net/10092/4935.

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A survey of the theory of neutrino oscillations in dense matter and neutrino backgrounds is presented. We discuss collective neutrino systems using the gyroscopic pendulum analogy and describe the motion that results from self-induced parametric resonances. The effects of dense matter on the flavour oscillations of neutrinos are also detailed. This theory is applied to the case of continuous supernova neutrino spectra and explanations of the spectral swapping behaviour seen in numerical studies are summarized. The results of numerical simulations of supernova oscillations in turbulent supernova backgrounds are presented and discussed. We study the motion of two example supernova neutrino spectra and examine the differences in the dynamics and flavour evolution that results from adding turbulent fluctuations to the supernova matter background. We also investigate the effect that fluctuations in the neutrino density can have on the oscillation behaviour. We find that in general the final neutrino spectra emerging from the inner supernova regions are quite robust to fluctuations in the backgrounds in our model, while the intermediate dynamics can be very strongly altered. Some significant changes in the final spectra are also found to occur when the neutrino background density fluctuations are large. We give a detailed review of the resonant matter effects that determine the survival probabilities of atmospheric muon neutrinos. The differences between various Earth density models are described, and these models are then used to predict the flux of muon-type neutrino events in the Deep Core extension to the IceCube detector. We use recent results from the detector collaboration and build on previous work which considered the sensitivity of the detector to the mass hierarchy, and show that uncertainties in the Earth's density can have a significant influence on the event rates.

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4

Li, Chao Thorne Kip S. Thorne Kip S. Chen Yanbei Cooray Asantha. "Topics in theoretical astrophysics /". Diss., Pasadena, Calif. : California Institute of Technology, 2009. http://resolver.caltech.edu/CaltechETD:etd-10142008-155140.

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5

Noble, Patrick. "Stochastic processes in Astrophysics". Thesis, The University of Sydney, 2013. http://hdl.handle.net/2123/10013.

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This thesis makes two contributions to the solar literature. The first is the development and application of a formal statistical framework for describing short-term (daily) variation in the level of magnetic activity on the Sun. Modelling changes on this time-scale is important because rapid developments of magnetic structures on the sun have important consequences for the space weather experienced on Earth (Committee On The Societal & Economic Impacts Of Severe Space Weather Events, 2008). The second concerns how energetic particles released from the Sun travel through the solar wind. The contribution from this thesis is to resolve a mathematical discrepancy in theoretical models for the transport of charged particles.

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6

Gao, Shu. "Energy transport mechanisms in astrophysics". Bachelor's thesis, Alma Mater Studiorum - Università di Bologna, 2021. http://amslaurea.unibo.it/22758/.

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To enable humans to observe, understand, and analyze celestial bodies, celestial bodies must emit energy from themselves and transmit them to the earth through free space, such as light, gravitational waves, or other things. Therefore, humans can analyze the content of celestial bodies based on the obtained information to understand the universe. This process can be called the energy transport process. He has exerted an important role in the communication between the earth and the universe, and we will discuss the main energy transport mechanisms in the stellar atmosphere in detail.

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7

Oppermann, Niels. "Signal inference in Galactic astrophysics". Diss., lmu, 2013. http://nbn-resolving.de/urn:nbn:de:bvb:19-154689.

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8

Haddock, D. J. "Stellar masses and laboratory astrophysics". Thesis, University of Oxford, 1987. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.379945.

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9

Johnson, Colin Terence. "Fine structure transitions in astrophysics". Thesis, Queen's University Belfast, 1987. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.317096.

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10

Nicholson, Kerry Louise. "The astrophysics of LINER galaxies". Thesis, University College London (University of London), 1998. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.298427.

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Libri sul tema "Astrophysics"

1

Kundt, Wolfgang. Astrophysics: A new approach. 2^a ed. Berlin: Springer, 2005.

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2

Kundt, Wolfgang. Astrophysics. Berlin, Heidelberg: Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-662-04347-9.

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3

Spatschek, Karl-Heinz. Astrophysics. Berlin, Heidelberg: Springer Berlin Heidelberg, 2024. http://dx.doi.org/10.1007/978-3-662-66648-7.

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4

M, Peterson B., a cura di. Foundations of astrophysics. New York: Pearson Addison-Wesley, 2009.

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5

J, Frank. Accretion power in astrophysics. 2^a ed. Cambridge [England]: Cambridge University Press, 1992.

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6

Zelinka, Ivan, Massimo Brescia e Dalya Baron, a cura di. Intelligent Astrophysics. Cham: Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-65867-0.

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7

Somov, Boris V. Plasma Astrophysics. New York, NY: Springer New York, 2007. http://dx.doi.org/10.1007/978-0-387-68894-7.

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8

Benz, Arnold. Plasma Astrophysics. Dordrecht: Springer Netherlands, 1993. http://dx.doi.org/10.1007/978-94-011-2064-7.

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9

Muñoz Caro, Guillermo M., e Rafael Escribano, a cura di. Laboratory Astrophysics. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-90020-9.

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10

Léna, Pierre. Observational Astrophysics. Berlin, Heidelberg: Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-662-02554-3.

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Capitoli di libri sul tema "Astrophysics"

1

Shafer, Wade H. "Astrophysics". In Masters Theses in the Pure and Applied Sciences, 49. Boston, MA: Springer US, 1996. http://dx.doi.org/10.1007/978-1-4613-0393-0_5.

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2

Shafer, Wade H. "Astrophysics". In Masters Theses in the Pure and Applied Sciences, 40. Boston, MA: Springer US, 1997. http://dx.doi.org/10.1007/978-1-4615-5969-6_5.

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3

Mould, Richard A. "Astrophysics". In Basic Relativity, 349–91. New York, NY: Springer New York, 1994. http://dx.doi.org/10.1007/978-1-4612-4326-7_13.

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4

Shafer, Wade H. "Astrophysics". In Masters Theses in the Pure and Applied Sciences, 52. Boston, MA: Springer US, 1992. http://dx.doi.org/10.1007/978-1-4615-3412-9_5.

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5

Shafer, Wade H. "Astrophysics". In Masters Theses in the Pure and Applied Sciences, 64. Boston, MA: Springer US, 1992. http://dx.doi.org/10.1007/978-1-4615-3474-7_5.

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6

Shafer, Wade H. "Astrophysics". In Masters Theses in the Pure and Applied Sciences, 59. Boston, MA: Springer US, 1989. http://dx.doi.org/10.1007/978-1-4613-0599-6_5.

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7

Shafer, Wade H. "Astrophysics". In Masters Theses in the Pure and Applied Sciences, 63. Boston, MA: Springer US, 1986. http://dx.doi.org/10.1007/978-1-4684-5197-9_5.

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8

Shafer, Wade H. "Astrophysics". In Masters Theses in the Pure and Applied Sciences, 47. Boston, MA: Springer US, 1993. http://dx.doi.org/10.1007/978-1-4615-2832-6_5.

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9

Flügge, S. "Astrophysics". In General Index / Generalregister, 667–734. Berlin, Heidelberg: Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-642-82502-6_11.

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10

Shafer, Wade H. "Astrophysics". In Masters Theses in the Pure and Applied Sciences, 37. Boston, MA: Springer US, 1997. http://dx.doi.org/10.1007/978-1-4757-5782-8_5.

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Atti di convegni sul tema "Astrophysics"

1

Rosner, R., J. Dursi, B. Fryxell, D. Lamb, C. Litwin, J. Niemeyer, K. Olson, H. Tufo e Y. Young. "Connecting astrophysics to laboratory fluid dynamics - Astrophysical thermonuclear flashes". In 30th Fluid Dynamics Conference. Reston, Virigina: American Institute of Aeronautics and Astronautics, 1999. http://dx.doi.org/10.2514/6.1999-3649.

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2

Kokhirova, G., P. Levkina, N. Bakhtigaraev e U. Khamroev. "Facilities of astrophysical telescopes in space debris research". 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/vak2021.2022.1.1.025.

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The possibilities of astrophysical telescopes for space debris research are shown. Some results of observations of space debris’fragments using the Zeiss–2000 telescope (D = 2 m, F = 16 m) Terskol branch of the Institute of Astronomy of the RussianAcademy of Sciences and Zeiss–1000 (D = 1 m, F = 13 m) of the Sanglokh observatory of the Institute of Astrophysics ofthe National academy of Sciences of Tajikistan are presented.

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3

Salamida, Francesco, e Irene Tamborra. "Multimessenger Astrophysics". In Neutrino Oscillation Workshop. Trieste, Italy: Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.283.0057.

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4

BOMBACI, IGNAZIO. "NUCLEAR ASTROPHYSICS". In Proceedings of the 9th Conference on Problems in Theoretical Nuclear Physics. WORLD SCIENTIFIC, 2003. http://dx.doi.org/10.1142/9789812705143_0003.

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5

Kundt, Wolfgang. "Gravitational Astrophysics". In Frontier Research in Astrophysics – III. Trieste, Italy: Sissa Medialab, 2018. http://dx.doi.org/10.22323/1.331.0016.

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6

Meyer, Mikko, e Kai Zuber. "Nuclear Astrophysics". In 5th International Solar Neutrino Conference. WORLD SCIENTIFIC, 2019. http://dx.doi.org/10.1142/9789811204296_others04.

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VIGEZZI, E. "NUCLEAR ASTROPHYSICS". In Proceedings of the 11th Conference on Problems in Theoretical Nuclear Physics. WORLD SCIENTIFIC, 2007. http://dx.doi.org/10.1142/9789812708793_0015.

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8

Haxton, W. C. "Nuclear Astrophysics". In INTERSECTIONS OF PARTICLE AND NUCLEAR PHYSICS: 9th Conference CIPAN2006. AIP, 2006. http://dx.doi.org/10.1063/1.2402595.

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DRAGO, ALESSANDRO. "NUCLEAR ASTROPHYSICS". In Proceedings of the 10th Conference on Problems in Theoretical Nuclear Physics. WORLD SCIENTIFIC, 2005. http://dx.doi.org/10.1142/9789812701985_0009.

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10

BRUNE, C. R. "NUCLEAR ASTROPHYSICS". In Proceedings of the Nineteenth Lake Louise Winter Institute. WORLD SCIENTIFIC, 2005. http://dx.doi.org/10.1142/9789812701961_0001.

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Rapporti di organizzazioni sul tema "Astrophysics"

1

Miller, Jonah. Nuclear Astrophysics and Astrophysical Transients. Office of Scientific and Technical Information (OSTI), novembre 2022. http://dx.doi.org/10.2172/1900461.

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2

Kamionkowski, Marc. Theoretical Particle Astrophysics. Office of Scientific and Technical Information (OSTI), agosto 2013. http://dx.doi.org/10.2172/1089511.

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3

Li, Hui. Astrophysics/Cosmology Status Report. Office of Scientific and Technical Information (OSTI), agosto 2017. http://dx.doi.org/10.2172/1375895.

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4

Cooperstein, J. Nuclear astrophysics of supernovae. Office of Scientific and Technical Information (OSTI), gennaio 1988. http://dx.doi.org/10.2172/6034283.

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5

Penionzhkevich, Yu E. Nuclear reactions in astrophysics. Physico-Technical Society of Kazakhstan, dicembre 2017. http://dx.doi.org/10.29317/ejpfm.2017010202.

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6

Schramm, D. N., e A. V. Olinto. Nuclear physics and astrophysics. Office of Scientific and Technical Information (OSTI), settembre 1992. http://dx.doi.org/10.2172/7073919.

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Ng, J. Accelerator Experiments for Astrophysics. Office of Scientific and Technical Information (OSTI), ottobre 2003. http://dx.doi.org/10.2172/826449.

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8

Burrows, Adam. SciDAC Computational Astrophysics Consortium. Office of Scientific and Technical Information (OSTI), giugno 2008. http://dx.doi.org/10.2172/932228.

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9

Intrator, Thomas P. Two LANL laboratory astrophysics experiments. Office of Scientific and Technical Information (OSTI), gennaio 2014. http://dx.doi.org/10.2172/1116693.

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10

Strait, Matthew, e Oleg Samoylov. The Astrophysics Program of NOvA. Office of Scientific and Technical Information (OSTI), giugno 2020. http://dx.doi.org/10.2172/1637609.

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