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Books on the topic 'Dynamics of the holes'

Author: Grafiati

Published: 4 June 2021

Last updated: 1 February 2022

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1

Aretakis, Stefanos. Dynamics of Extremal Black Holes. Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-95183-6.

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2

Hemsendorf, Marc. Dynamics of black holes in galactic centres. Shaker, 2000.

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3

MHD flows in compact astrophysical objects: Accretion, winds and jets. Springer, 2010.

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4

Sachar, Louis. Holes. Scholastic, 2000.

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5

Sachar, Louis. Holes. Scholastic Inc., 1999.

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6

Sachar, Louis. Holes. Holt, Rinehart and Winston, 2002.

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7

Sachar, Louis. Holes. Scholastic, 2000.

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8

Sachar, Louis. Holes. Farrar, Straus and Giroux, 2008.

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9

Sachar, Louis. Holes. Scholastic Inc., 1999.

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10

ill, Shott Stephen, ed. Holes. Childrens Press, 1995.

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11

Sachar, Louis. Holes. Bloomsbury, 2007.

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12

Sachar, Louis. Holes. Bloomsbury, 2002.

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13

Sachar, Louis. Holes. Dell Yearling, 2000.

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14

Sachar, Louis. Holes. Thorndike Press, 1999.

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15

Sachar, Louis. Holes. Farrar, Straus and Giroux, 1998.

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16

Sachar, Louis. Holes. Dell Laurel-Leaf, 2001.

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17

Black holes. PowerKids Press, 1997.

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18

Rau, Dana Meachen. Black holes. Compass Point Books, 2005.

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19

Luminet, Jean-Pierre. Black holes. Cambridge University Press, 1992.

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20

Sachar, Louis. Ana =: Holes. K̄dansha, 1999.

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21

Than, Ker. Black holes. Children's Press, 2010.

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22

Black holes. Stanford University Press, 1999.

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23

Sipiera, Paul P. Black holes. Children's Press, 1997.

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24

Black holes. Capstone Press, 2012.

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25

ill, Marshall Felicia, ed. Secret holes. Carolrhoda Books, 2003.

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26

Sachar, Louis. Dong: Holes. Nan Hai chu ban gong si, 2014.

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27

Black holes. ABDO Pub., 2011.

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28

Aretakis, Stefanos. Dynamics of Extremal Black Holes. Springer, 2018.

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29

Dynamics and Evolution of Galactic Nuclei. Princeton University Press, 2013.

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30

Merritt, David. Dynamics and Evolution of Galactic Nuclei. Princeton University Press, 2013.

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31

Chruściel, Piotr T. Geometry of Black Holes. Oxford University Press, 2020. http://dx.doi.org/10.1093/oso/9780198855415.001.0001.

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There exists a large scientific literature on black holes, including many excellent textbooks of various levels of difficulty. However, most of these prefer physical intuition to mathematical rigour. The object of this book is to fill this gap and present a detailed, mathematically oriented, extended introduction to the subject. The first part of the book starts with a presentation, in Chapter 1, of some basic facts about Lorentzian manifolds. Chapter 2 develops those elements of Lorentzian causality theory which are key to the understanding of black-hole spacetimes. We present some applicatio

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32

Keszthelyi, Bettina E. Gravitational models in 2+1 dimensions with topological terms and thermo-field dynamics of black holes. 1993.

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33

(Editor), Maurice M. Shapiro, Todor Stanev (Editor), and John P. Wefel (Editor), eds. Neutrinos and Explosive Events in the Universe: Proceedings of the NATO Advanced Study Institute, held in Erice, Italy, 2-13 July 2004 (NATO Science Series II: Mathematics, Physics and Chemistry, Vol. 209). Springer, 2005.

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34

R, Genzel, Harris A. I, and NATO Advanced Research Workshop on the Nuclei of Normal Galaxies (1993 : Kreuth, Germany), eds. The nuclei of normal galaxies: Lessons from the Galactic Center. Kluwer Academic, 1994.

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35

(Editor), R. Genzel, and Andrew I. Harris (Editor), eds. The Nuclei of Normal Galaxies: Lessons from the Galactic Center (NATO Science Series C: Mathematical and Physical Sciences, Volume 445). Kluwer Academic, 1994.

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36

Genzel, R. The Nuclei of Normal Galaxies: Lessons From The Galactic Center. Ingramcontent, 2012.

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37

Blundell, Katherine. 6. How do you weigh a black hole? Oxford University Press, 2015. http://dx.doi.org/10.1093/actrade/9780199602667.003.0006.

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Infra-red observations have been used by teams in California and Germany to measure the mass of the black hole at the centre of the Galaxy at just over 4 million times the mass of our Sun. ‘How do you weigh a black hole?’ shows that similar dynamic techniques can be used to measure the masses of the millions of black holes that pervade our Galaxy as stars and black holes are frequently found as pairs in a binary system. The smallest black hole that we can measure is a few times the mass of our Sun, but the heaviest stellar-mass black holes can exceed a hundred times the mass of our Sun.

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38

(Editor), Maurice M. Shapiro, Todor Stanev (Editor), and John P. Wefel (Editor), eds. Neutrinos and Explosive Events in the Universe (NATO Science Series II: Mathematics, Physics and Chemistry). Springer, 2005.

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39

Glazov, M. M. Electron & Nuclear Spin Dynamics in Semiconductor Nanostructures. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198807308.001.0001.

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In recent years, the physics community has experienced a revival of interest in spin effects in solid state systems. On one hand, solid state systems, particularly semicon- ductors and semiconductor nanosystems, allow one to perform benchtop studies of quantum and relativistic phenomena. On the other hand, interest is supported by the prospects of realizing spin-based electronics where the electron or nuclear spins can play a role of quantum or classical information carriers. This book aims at rather detailed presentation of multifaceted physics of interacting electron and nuclear spins in sem

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40

Nolte, David D. Flight of the Swallows. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198805847.003.0001.

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The science of modern dynamics takes the simple idea of Galileo’s parabolic trajectory and generalizes it into abstract hyperspaces of multiple dimensions. This chapter introduces the new way that physicists and mathematicians visualize dynamical systems, taking a global view of complex behavior and finding that the laws of physics capture the orbits of planets around suns (and the paths of light around black holes) as easily as the evolution of new species or the rise and fall of economies. This new visualization uses phase space to capture the global behavior of complex systems. The path acr

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41

Glazov, M. M. Hyperfine Interaction of Electron and Nuclear Spins. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198807308.003.0004.

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This chapter discusses the key interaction–hyperfine coupling–which underlies most of phenomena in the field of electron and nuclear spin dynamics. This interaction originates from magnetic interaction between the nuclear and electron spins. For conduction band electrons in III–V or II–VI semiconductors, it is reduced to a Fermi contact interaction whose strength is proportional to the probability of finding an electron at the nucleus. A more complex situation is realized for valence band holes where hole Bloch functions vanish at the nuclei. Here the hyperfine interaction is of the dipole–dip

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42

Deruelle, Nathalie, and Jean-Philippe Uzan. The two-body problem: an effective-one-body approach. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198786399.003.0056.

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This chapter presents the basics of the ‘effective-one-body’ approach to the two-body problem in general relativity. It also shows that the 2PN equations of motion can be mapped. This can be done by means of an appropriate canonical transformation, to a geodesic motion in a static, spherically symmetric spacetime, thus considerably simplifying the dynamics. Then, including the 2.5PN radiation reaction force in the (resummed) equations of motion, this chapter provides the waveform during the inspiral, merger, and ringdown phases of the coalescence of two non-spinning black holes into a final Ke

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43

Claster, Daniel S., and Howard W. Polsky. Dynamics of Residential Treatment: A Social System Analysis. University of North Carolina Press, 2012.

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44

Saha, Prasenjit, and Paul A. Taylor. Schwarzschild’s Spacetime. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198816461.003.0003.

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The concept of a metric is motivated and introduced, along with the introduction of relativistic quantities of spacetime, proper time, and Einstein’s field equations. Geodesics are cast in basic form as a Hamiltonian dynamical problem, which readers are guided towards exploring numerically themselves. The specific case of the Schwarzschild metric is presented, which is applicable to space around non-rotating black holes, and orbital motion around such objects is contrasted with that of Newtonian systems. Some well-known formulas for black hole phenomena are derived, such as those for light def

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45

Holes. HarperCollins Publishers, 1990.

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46

Sachar, Louis. Holes. Bolinda/Audible audio, 2018.

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47

Dreibrodt, Stacie Champlin. Holes. Novel Units, 1999.

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48

Beyer, Kerry. Holes. Listening Library, 2006.

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49

Sachar, Louis. Holes. Listening Library, 1999.

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50

Sachar, Louis. Holes. Bloomsbury Publishing PLC, 2000.

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