Academic literature on the topic 'Particle Astrophyics'

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Journal articles on the topic "Particle Astrophyics"

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Barzi, E., G. Bellettini, S. Donati, and D. Pasciuto. "Involving the new generations in particle physics endeavours." Journal of Physics: Conference Series 2156, no. 1 (2021): 012160. http://dx.doi.org/10.1088/1742-6596/2156/1/012160.

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Abstract Since 1984 INFN and University of Pisa scientists performing experiments at Fermilab have been running a two-month summer training program for Italian students at the lab. In 1984 the program involved only a few physics students from the University of Pisa, but it was later extended to other INFN groups and to engineering students. Since 2004 the program has been supported in part by the US Department of Energy (DOE) in the frame of an exchange agreement with INFN and has been run by the Cultural Association of Italians at Fermilab (CAIF). In 2007 the Sant’Anna School of Advanced Stud
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Auriemma, Giulio. "LHC, Astrophysics and Cosmology." Acta Polytechnica CTU Proceedings 1, no. 1 (2014): 42–48. http://dx.doi.org/10.14311/app.2014.01.0042.

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In this paper we discuss the impact on cosmology of recent results obtained by the LHC (Large Hadron Collider) experiments in the 2011-2012 runs, respectively at √<span style="text-decoration: overline;">s</span> = 7 and 8 TeV. The capital achievement of LHC in this period has been the discovery of a spin-0 particle with mass 126 GeV/c<sup>2</sup>, very similar to the Higgs boson of the Standard Model of Particle Physics. Less exciting, but not less important, negative results of searches for Supersymmetric particles or other exotica in direct production or rare decays
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CHATELAIN, PHILIPPE, GEORGES-HENRI COTTET, and PETROS KOUMOUTSAKOS. "PARTICLE MESH HYDRODYNAMICS FOR ASTROPHYSICS SIMULATIONS." International Journal of Modern Physics C 18, no. 04 (2007): 610–18. http://dx.doi.org/10.1142/s0129183107010851.

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We present a particle method for the simulation of three dimensional compressible hydrodynamics based on a hybrid Particle-Mesh discretization of the governing equations. The method is rooted on the regularization of particle locations as in remeshed Smoothed Particle Hydrodynamics (rSPH). The rSPH method was recently introduced to remedy problems associated with the distortion of computational elements in SPH, by periodically re-initializing the particle positions and by using high order interpolation kernels. In the PMH formulation, the particles solely handle the convective part of the comp
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Gaisser, Thomas K. "Particle astrophysics." Nuclear Physics B - Proceedings Supplements 117 (April 2003): 318–34. http://dx.doi.org/10.1016/s0920-5632(03)01425-7.

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Battiston, R. "Particle astrophysics." Advances in Space Research 37, no. 10 (2006): 1833. http://dx.doi.org/10.1016/j.asr.2006.03.014.

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Sadouler, Bernard, and James W. Cronin. "Particle Astrophysics." Physics Today 44, no. 4 (1991): 53–57. http://dx.doi.org/10.1063/1.881288.

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Klapdor‐Kleingrothaus, Hans V., Kai Zuber, and Bernard Sadoulet. "Particle Astrophysics." Physics Today 51, no. 11 (1998): 66–69. http://dx.doi.org/10.1063/1.882058.

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Protheroe, R. J., and R. W. Clay. "Ultra High Energy Cosmic Rays." Publications of the Astronomical Society of Australia 21, no. 1 (2004): 1–22. http://dx.doi.org/10.1071/as03047.

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AbstractCosmic rays with energies above 1018 eV are currently of considerable interest in astrophysics and are to be further studied in a number of projects which are either currently under construction or the subject of well-developed proposals. This paper aims to discuss some of the physics of such particles in terms of current knowledge and information from particle astrophysics at other energies.
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Dröge, Wolfgang. "Particle Acceleration by Waves and Fields." Highlights of Astronomy 11, no. 2 (1998): 865–68. http://dx.doi.org/10.1017/s1539299600018967.

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The acceleration of electrons and charged nuclei to high energies is a phenomenon occuring at many sites throughout the universe, including the galaxy, pulsars, quasars, and around black holes. In the heliosphere, large solar flares and the often associated coronal mass ejections (CMEs) are the most energetic natural particle accelerators, occasionally accelerating protons to GeV and electrons to tens of MeV energies. The observation of these particles offers the unique opportunity to study fundamental processes in astrophysics. Particles that escape into interplanetary space can be observed i
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Bergström, Lars, Ariel Goobar, and Andrew H. Jaffe. "Cosmology and Particle Astrophysics." American Journal of Physics 69, no. 3 (2001): 394. http://dx.doi.org/10.1119/1.1336841.

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Dissertations / Theses on the topic "Particle Astrophyics"

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Todd, Elizabeth. "Particle Astrophysics at the Galactic Center." Diss., The University of Arizona, 2011. http://hdl.handle.net/10150/145121.

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The presence of turbulence in astrophysical magnetic fields can have a significant effect on the diffusion of particles and, therefore, should be taken into account when performing simulations involving particle propagation. After reviewing the constructionof the turbulent magnetic field component, we incorporate this feature in two separate projects. In the first, we consider the possible source(s) of hadronic cosmic rays thought to be responsible for the diffuse TeV gamma-ray emission in the vicinity ofthe Galactic center. Assuming a completely turbulent magnetic field with an average streng
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Feroz, Farhan. "Bayesian methods for astrophysics and particle physics." Thesis, University of Cambridge, 2008. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.612370.

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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 superno
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Banerjee, Oindree. "Studies in particle astrophysics with the ANITA experiment." The Ohio State University, 2018. http://rave.ohiolink.edu/etdc/view?acc_num=osu1532097132391735.

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Walker, Richard Thomas. "Computational Steering of Smoothed Particle Hydrodynamics Simulations for Astrophysics." Thesis, University of Kent, 2009. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.499677.

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Powell, Andrew James. "The cosmology and astrophysics of axion-like particles." Thesis, University of Oxford, 2016. https://ora.ox.ac.uk/objects/uuid:bbbb3cbc-a0ba-4024-86b0-c720d8104270.

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In this thesis I study astrophysical and cosmological effects of axion-like particles (ALPs). ALPs are pseudo-scalar particles, which are generally very weakly-interacting, with a coupling α/M E · B to electromagnetism. They are predicted by many theories which extend the standard model (SM) of particle physics, most notably string theory. String theory compactifications also predict many scalar fields called moduli which describe the size and shape of the extra, compact dimensions. In string theory models generically the moduli fields are responsible for reheating the universe after inflation
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Grieb, Christian. "Future neutrino detectors and their impact on particle- and astrophysics." [S.l. : s.n.], 2004. http://deposit.ddb.de/cgi-bin/dokserv?idn=973900261.

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Eby, Joshua. "Phenomenology and Astrophysics of Gravitationally-Bound Condensates of Axion-Like Particles." University of Cincinnati / OhioLINK, 2017. http://rave.ohiolink.edu/etdc/view?acc_num=ucin1504868633515325.

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DI, PIAZZA ANTONINO. "PARTICLE PRODUCTION IN A STRONG, SLOWLY-VARYING MAGNETIC FIELD WITH AN APPLICATION TO ASTROPHYSICS." Doctoral thesis, Università degli studi di Trieste, 2004. http://thesis2.sba.units.it/store/handle/item/12549.

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2002/2003<br>In questo lavoro ho affrontato lo studio della produzione dal vuoto di particelle (elettroni, posi troni e fotoni) in presenza di campi magnetici intensi e lentamente variabili nel tempo. Per "campi magnetici intensi" intendo campi magnetici la cui intensità è molto maggiore del valore Ber = m2c3 /(ne) = 4.4 x 1013 gauss che corrisponde al valore minimo dell'ampiezza che un campo magnetico deve avere affinché risulti energeticamente possibile la creazione dal vuoto di una coppia e- - e+. Tali campi magnetici non possono essere prodotti in laboratorio, tuttavia, come mostrano certe
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Phelps, Patrick. "THE LUX DARK MATTER EXPERIMENT: DETECTOR PERFORMANCE AND ENERGY CALIBRATION." Case Western Reserve University School of Graduate Studies / OhioLINK, 2014. http://rave.ohiolink.edu/etdc/view?acc_num=case1404908222.

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Books on the topic "Particle Astrophyics"

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Particle astrophysics. Institute of Physics Pub., 2000.

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G, Fontaine, Tran J. Thanh Van, Comité national de la recherche scientifique (France), and Rencontres de Blois (4th : 1992 : Château de Blois), eds. Particle astrophysics. Editions Frontieres, 1993.

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Particle astrophysics. 2nd ed. Oxford University Press, 2008.

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Particle astrophysics. Oxford University Press, 2003.

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Klapdor-Kleingrothaus, H. V. Particle astrophysics. Institute of Physics Publ., 1997.

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Perkins, Donald H. Particle astrophysics. 2nd ed. Oxford University Press, 2009.

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Shapiro, Maurice M., Rein Silberberg, and John P. Wefel, eds. Particle Astrophysics and Cosmology. Springer Netherlands, 1993. http://dx.doi.org/10.1007/978-94-011-1707-4.

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1915-, Shapiro Maurice M., Silberberg Rein 1932-, and Wefel J. P, eds. Particle astrophysics and cosmology. Kluwer Academic Publishers, 1993.

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Shapiro, Maurice M. Particle Astrophysics and Cosmology. Springer Netherlands, 1993.

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Bergstrom, L. (Lars). Cosmology and particle astrophysics. 2nd ed. PRAXIS PUBLISHING (UK), 2004.

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Book chapters on the topic "Particle Astrophyics"

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Koskinen, Hannu E. J., and Emilia K. J. Kilpua. "From Charged Particles to Plasma Physics." In Astronomy and Astrophysics Library. Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-82167-8_3.

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AbstractIn this chapter we move from single particle motion to the statistical description of a large number of charged particles, the plasma. This discussion provides the basis for the rich flora of plasma waves that are essential for understanding the sources and losses of radiation belt particles through wave–particle interactions.
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Koskinen, Hannu E. J., and Emilia K. J. Kilpua. "Charged Particles in Near-Earth Space." In Astronomy and Astrophysics Library. Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-82167-8_2.

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AbstractIn this chapter we discuss the concepts that govern the motion of charged particles in the geomagnetic field and the principles how they stay trapped in the radiation belts. The basic particle orbit theory can be found in most plasma physics textbooks. We partly follow the presentation in Koskinen (Physics of space storms, from solar surface to the earth. Springer-Praxis, Heidelberg, 2011). A more detailed discussion can be found in Roederer and Zhang (Dynamics of magnetically trapped particles. Springer, Heidelberg, 2014). A classic treatment of adiabatic motion of charged particles is Northrop (The adiabatic motion of charged particles. Interscience Publishers, Wiley, New York, 1963).
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Achterberg, A. "Particle acceleration in astrophysics." In Galactic High-Energy Astrophysics High-Accuracy Timing and Positional Astronomy. Springer Berlin Heidelberg, 1993. http://dx.doi.org/10.1007/3-540-56874-3_1.

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Drury, Luke O’C. "Particle Acceleration in Astrophysics." In Nuclei Far from Stability and Astrophysics. Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-010-0708-5_29.

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Schatzman, E. "Particle Physics and Astrophysics." In Springer Proceedings in Physics. Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-642-73473-1_50.

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Koskinen, Hannu E. J., and Emilia K. J. Kilpua. "Particle Source and Loss Processes." In Astronomy and Astrophysics Library. Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-82167-8_6.

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AbstractThe main sources of charged particles in the Earth’s inner magnetosphere are the Sun and the Earth’s ionosphere. Furthermore, the Galactic cosmic radiation is an important source of protons in the inner radiation belt, and roughly every 13 years, when the Earth and Jupiter are connected via the interplanetary magnetic field, a small number of electrons originating from the magnetosphere of Jupiter are observed in the near-Earth space. The energies of solar wind and ionospheric plasma particles are much smaller than the particle energies in radiation belts. A major scientific task is to understand the transport and acceleration processes leading to the observed populations up to relativistic energies. Equally important is to understand the losses of the charged particles. The great variability of the outer electron belt is a manifestation of the continuously changing balance between source and loss mechanisms, whereas the inner belt is much more stable.
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Silberberg, R., M. M. Shapiro, and C. H. Starr. "Neutrino and Gamma-Ray Astrophysics." In Particle Astrophysics and Cosmology. Springer Netherlands, 1993. http://dx.doi.org/10.1007/978-94-011-1707-4_6.

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Berezinsky, V. "Puzzles in Astrophysics." In Cosmic Radiations: From Astronomy to Particle Physics. Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-010-0634-7_1.

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Koskinen, Hannu E. J., and Emilia K. J. Kilpua. "Plasma Waves in the Inner Magnetosphere." In Astronomy and Astrophysics Library. Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-82167-8_4.

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AbstractUnderstanding the role of plasma waves, extending from magnetohydrodynamic (MHD) waves at ultra-low-frequency (ULF) oscillations in the millihertz range to very-low-frequency (VLF) whistler-mode emissions at frequencies of a few kHz, is necessary in studies of sources and losses of radiation belt particles. In order to make this theoretically heavy part of the book accessible to a reader, who is not familiar with wave–particle interactions, we have divided the treatise into three chapters. In the present chapter we introduce the most important wave modes that are critical to the dynamics of radiation belts. The drivers of these waves are discussed in Chap. 10.1007/978-3-030-82167-8_5 and the roles of the wave modes as sources and losses of radiation belt particles are dealt with in Chap. 10.1007/978-3-030-82167-8_6.
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Monaghan, J. J. "Smoothed Particle Hydrodynamics." In Numerical Astrophysics. Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4780-4_110.

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Conference papers on the topic "Particle Astrophyics"

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Carr, John. "Particle astrophysics." In International Europhysics Conference on High Energy Physics. Sissa Medialab, 2001. http://dx.doi.org/10.22323/1.007.0300.

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Sonnenschein, Andrew. "Experimental Particle Astrophysics." In Experimental Particle Astrophysics. US DOE, 2008. http://dx.doi.org/10.2172/1967454.

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Ramaty, R., R. J. Murphy, and J. A. Miller. "Solar accelerated particles: Comparisons of abundances and energy spectra from particle and gamma-ray observations." In Particle astrophysics. AIP, 1990. http://dx.doi.org/10.1063/1.39147.

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Dine, Michael. "Particle astrophysics from the particle perspective." In The XVI international sympsosium on lepton and photon interactions. AIP, 1994. http://dx.doi.org/10.1063/1.45469.

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Price, P. B. "Heavy nucleus collector for space station." In Particle astrophysics. AIP, 1990. http://dx.doi.org/10.1063/1.39142.

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Smoot, George F. "The Astromag facility." In Particle astrophysics. AIP, 1990. http://dx.doi.org/10.1063/1.39143.

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Cherry, Michael L. "Cosmic rays above 1 TeV/n and neutrino astronomy (Splinter group summary)." In Particle astrophysics. AIP, 1990. http://dx.doi.org/10.1063/1.39158.

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Wiedenbeck, Mark E. "The abundances of ultraheavy nuclei in solar energetic particles." In Particle astrophysics. AIP, 1990. http://dx.doi.org/10.1063/1.39159.

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Swordy, Simon P. "A ring imaging Čerenkov counter for Astromag to study the isotopic composition of cosmic rays." In Particle astrophysics. AIP, 1990. http://dx.doi.org/10.1063/1.39160.

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Cherry, Michael L. "Neutrino astronomy on the moon—practical considerations." In Particle astrophysics. AIP, 1990. http://dx.doi.org/10.1063/1.39130.

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Reports on the topic "Particle Astrophyics"

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

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Nitz, David F., and Brian E. Fick. Studies of High Energy Particle Astrophysics. Office of Scientific and Technical Information (OSTI), 2014. http://dx.doi.org/10.2172/1145912.

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Wagner, R. G., K. L. Byrum, M. Sanchez, et al. The next generation of photo-detector for particle astrophysics. Office of Scientific and Technical Information (OSTI), 2009. http://dx.doi.org/10.2172/956926.

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Kearns, Edward. Research in Neutrino Physics and Particle Astrophysics: Final Technical Report. Office of Scientific and Technical Information (OSTI), 2016. http://dx.doi.org/10.2172/1259746.

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Starkman, Glenn David, and Harsh Mathur. Particle Astrophysics Theory Group, CWRU 2013 Final Report on DOE grant. Office of Scientific and Technical Information (OSTI), 2013. http://dx.doi.org/10.2172/1087735.

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Chen, P. Workshop on Laboratory Astrophysics Using High Intensity Particle and Photon Beams. Office of Scientific and Technical Information (OSTI), 2003. http://dx.doi.org/10.2172/826575.

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Eby, Joshua Armstrong. Phenomenology and Astrophysics of Gravitationally-Bound Condensates of Axion-Like Particles. Office of Scientific and Technical Information (OSTI), 2017. http://dx.doi.org/10.2172/1408206.

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Matthews, John, Sally Seidel, and Michael Gold. New Mexico Center for Particle Physics (NMCPP) -- Task A: Collider Physics; Task A2: Collider Physics; Task B: Particle Astrophysics. Office of Scientific and Technical Information (OSTI), 2013. http://dx.doi.org/10.2172/1098244.

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Lyons, L. Proceedings of the Conference on Statistical Problems for Particle Physics, Astrophysics and Cosmology (PHYSTAT2003). Office of Scientific and Technical Information (OSTI), 2004. http://dx.doi.org/10.2172/826884.

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Nitz, David F., and Brian E. Fick. Final Report for DoE Grant DE-SC-0011689 - Studies of Particle Astrophysics at the Cosmic Frontier. Office of Scientific and Technical Information (OSTI), 2016. http://dx.doi.org/10.2172/1252987.

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