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1

Peter, Mészáros, Begelman Mitchell C i United States. National Aeronautics and Space Administration., red. Why 'galactic' gamma-ray bursts might depend on environment: Blast waves around neutron stars. [Washington, DC: National Aeronautics and Space Administration, 1994.

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2

Peter, Mészáros, Begelman Mitchell C i United States. National Aeronautics and Space Administration., red. Why 'galactic' gamma-ray bursts might depend on environment: Blast waves around neutron stars. [Washington, DC: National Aeronautics and Space Administration, 1994.

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3

Peter, Mészáros, Begelman Mitchell C i United States. National Aeronautics and Space Administration., red. Why 'galactic' gamma-ray bursts might depend on environment: Blast waves around neutron stars. [Washington, DC: National Aeronautics and Space Administration, 1994.

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4

International, School on Nuclear Physics Neutron Physics and Nuclear Energy (8th 1987 Varna Bulgaria). Nuclei, neutrons, and energy: Proceedings of the VIII International School on Nuclear Physics, Neutron Physics, and Nuclear Energy, Varna, Bulgaria, 19-28 Nov. 1987. Singapore: World Scientific, 1988.

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5

Rubinstein, Robert. Non-ideal gas effects on shock waves in weakly ionized gases. Hampton, VA: Institute for Computer Applications in Science and Engineering, NASA Langley Research Center, 2000.

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6

Rubinstein, Robert. Non-ideal gas effects on shock waves in weakly ionized gases. Hampton, VA: Institute for Computer Applications in Science and Engineering, NASA Langley Research Center, 2000.

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7

Rubinstein, Robert. Non-ideal gas effects on shock waves in weakly ionized gases. Hampton, VA: Institute for Computer Applications in Science and Engineering, NASA Langley Research Center, 2000.

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8

Rubinstein, Robert. Non-ideal gas effects on shock waves in weakly ionized gases. Hampton, VA: Institute for Computer Applications in Science and Engineering, NASA Langley Research Center, 2000.

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9

Rubinstein, Robert. Non-ideal gas effects on shock waves in weakly ionized gases. Hampton, VA: Institute for Computer Applications in Science and Engineering, NASA Langley Research Center, 2000.

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10

Rubinstein, Robert. Non-ideal gas effects on shock waves in weakly ionized gases. Hampton, VA: Institute for Computer Applications in Science and Engineering, NASA Langley Research Center, 2000.

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11

Rubinstein, Robert. Non-ideal gas effects on shock waves in weakly ionized gases. Hampton, VA: Institute for Computer Applications in Science and Engineering, NASA Langley Research Center, 2000.

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12

Kursunoglu, Behram N., Stephan L. Mintz i Arnold Perlmutter, red. Neutrino Mass, Dark Matter, Gravitational Waves, Monopole Condensation, and Light Cone Quantization. Boston, MA: Springer US, 1996. http://dx.doi.org/10.1007/978-1-4899-1564-1.

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13

1922-, Kurşunoğlu Behram, Mintz Stephan L, Perlmutter Arnold 1928- i International Conference on Orbis Scientiae (1996 : Miami Beach, Fla.), red. Neutrino mass, dark matter, gravitational waves, monopole condensation, and light cone quantization. New York: Plenum Press, 1996.

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14

M, Elcombe M., Hicks T. J, New South Wales Institute of Technology. i International Union of Crystallography, red. Neutron scattering advances and applications: Proceedings of a symposium held at the New South Wales Institute of Technology, Sydney, Australia, August 8-11, 1987. Aedermannsdorf, Switzerland: Trans Tech Publications, 1988.

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15

Baykal, Altan, Sinan K. Yerli, Sitki C. Inam i Sergei Grebenev. Electromagnetic Spectrum of Neutron Stars. Springer, 2005.

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16

Kolata, James J. Neutron Stars, Black Holes, and Gravitational Waves. Morgan & Claypool Publishers, 2019.

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17

Kolata, James J. Neutron Stars, Black Holes, and Gravitational Waves. Morgan & Claypool Publishers, 2019.

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18

Kolata, James J. Neutron Stars, Black Holes, and Gravitational Waves. Morgan & Claypool Publishers, 2019.

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19

Dubovichenko, Sergey Borisovich. Radiative Neutron Capture: Primordial Nucleosynthesis of the Universe. De Gruyter, Inc., 2019.

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20

Dubovichenko, Sergey Borisovich. Radiative Neutron Capture: Primordial Nucleosynthesis of the Universe. de Gruyter GmbH, Walter, 2019.

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21

Dubovichenko, Sergey Borisovich. Radiative Neutron Capture: Primordial Nucleosynthesis of the Universe. de Gruyter GmbH, Walter, 2019.

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22

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, GW151226, tests of general relativity, astrophysical implications), supermassive black holes (supermassive black-hole binaries, EMRI, relevance for LISA and pulsar timing arrays). The part on gravitational waves and cosmology include discussions of FRW cosmology, cosmological perturbation theory (helicity decomposition, scalar and tensor perturbations, Bardeen variables, power spectra, transfer functions for scalar and tensor modes), the effects of GWs on the Cosmic Microwave Background (ISW effect, CMB polarization, E and B modes), inflation (amplification of vacuum fluctuations, quantum fields in curved space, generation of scalar and tensor perturbations, Mukhanov-Sasaki equation,reheating, preheating), stochastic backgrounds of cosmological origin (phase transitions, cosmic strings, alternatives to inflation, bounds on primordial GWs) and search of stochastic backgrounds with Pulsar Timing Arrays (PTA).
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23

(Editor), Altan Baykal, Sinan K. Yerli (Editor), Sitki C. Inam (Editor) i Sergei Grebenev (Editor), red. The Electromagnetic Spectrum of Neutron Stars (NATO Science Series II: Mathematics, Physics and Chemistry). Springer, 2005.

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24

Fishman, Randy S., Jaime A. Fernandez-Baca i Toomas Rõõm. Spin-Wave Theory and Its Applications to Neutron Scattering and THz Spectroscopy. Morgan & Claypool Publishers, 2018.

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25

Fishman, Randy S., Jaime A. Fernandez-Baca i Toomas Rõõm. Spin-Wave Theory and Its Applications to Neutron Scattering and THz Spectroscopy. Morgan & Claypool Publishers, 2018.

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26

Fishman, Randy S., Jaime A. Fernandez-Baca i Toomas Rõõm. Spin-Wave Theory and Its Applications to Neutron Scattering and THz Spectroscopy. Morgan & Claypool Publishers, 2018.

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27

Kyutoku, Koutarou. Black Hole-Neutron Star Binary Merger in Full General Relativity: Dependence on Neutron Star Equations of State. Springer London, Limited, 2013.

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28

Kyutoku, Koutarou. The Black Hole-Neutron Star Binary Merger in Full General Relativity: Dependence on Neutron Star Equations of State. Springer, 2013.

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29

Kyutoku, Koutarou. The Black Hole-Neutron Star Binary Merger in Full General Relativity: Dependence on Neutron Star Equations of State. Springer, 2015.

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30

(Editor), D. Elenkov, red. Nuclei, Neutrons, and Energy: Proceedings of the VIII International School on Nuclear Physics, Neutron Physics, and Nuclear Energy. World Scientific Pub Co Inc, 1988.

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31

Braude, S. Ya, i V. M. Kontorovich. Radio Waves Tell About the Universe. PH “Akademperiodyka”, 2005. http://dx.doi.org/10.15407/akademperiodyka.005.279.

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The book tells about the achievements of modern radio astronomy. Data on radio galaxies, quasars, pulsars, space masers, and other space objects emitting radio waves are presented in a popular form. The ways of evolution of stars, supernovae and radio eruptions of their remains, the formation of white dwarfs and neutron stars, the phenomena in the centers of galaxies and the fusion of galaxies responsible for the formation of radio galaxies and quasars are considered. The radio radiation of the Sun and planets is discussed. A modern view of the evolution of the universe, the origin of the relic radiation left over from the Great Eruption, and its anisotropy is presented. A separate chapter is devoted to the description of radio telescopes.
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32

(Editor), Altan Baykal, Sinan K. Yerli (Editor), Sitki C. Inam (Editor) i Sergei Grebenev (Editor), red. The Electromagnetic Spectrum of Neutron Stars (NATO Science Series II: Mathematics, Physics and Chemistry, Vol. 210). Springer, 2005.

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33

Rotating Relativistic Stars. Cambridge University Press, 2008.

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34

Moffat, John W. The Shadow of the Black Hole. Oxford University Press, 2020. http://dx.doi.org/10.1093/oso/9780190650728.001.0001.

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The author visits one of the two Laser Interferometer Gravitational- Wave Observatory (LIGO) sites in the United States, at Hanford, Washington. This is where scientists are detecting gravitational waves generated by faraway merging black holes and neutron stars. He meets the people who work there and has discussions with some of them. The director gives him a tour of the LIGO experimental installation, describing the work, the technological details of the apparatus, and answers his questions. On the final day of the visit, the author gives a talk to the LIGO group on gravitational waves and on an alternative gravitational theory.
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35

Rauch, Helmut, i Samuel A. Werner. Neutron Interferometry: Lessons in Experimental Quantum Mechanics, Wave-Particle Duality, and Entanglement. Oxford University Press, 2018.

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36

Mee, Nicholas. The Cosmic Mystery Tour. Oxford University Press, 2019. http://dx.doi.org/10.1093/oso/9780198831860.001.0001.

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The Cosmic Mystery Tour is a brief account of modern physics and astronomy presented in a broad historical and cultural context. The book is attractively illustrated and aimed at the general reader. Part I explores the laws of physics including general relativity, the structure of matter, quantum mechanics and the Standard Model of particle physics. It discusses recent discoveries such as gravitational waves and the project to construct LISA, a space-based gravitational wave detector, as well as unresolved issues such as the nature of dark matter. Part II begins by considering cosmology, the study of the universe as a whole and how we arrived at the theory of the Big Bang and the expanding universe. It looks at the remarkable objects within the universe such as red giants, white dwarfs, neutron stars and black holes, and considers the expected discoveries from new telescopes such as the Extremely Large Telescope in Chile, and the Event Horizon Telescope, currently aiming to image the supermassive black hole at the galactic centre. Part III considers the possibility of finding extraterrestrial life, from the speculations of science fiction authors to the ongoing search for alien civilizations known as SETI. Recent developments are discussed: space probes to the satellites of Jupiter and Saturn; the discovery of planets in other star systems; the citizen science project SETI@Home; Breakthrough Starshot, the project to develop technologies to send spacecraft to the stars. It also discusses the Fermi paradox which argues that we might actually be alone in the cosmos
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37

Non-ideal gas effects on shock waves in weakly ionized gases. Hampton, VA: Institute for Computer Applications in Science and Engineering, NASA Langley Research Center, 2000.

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38

Andersson, Nils. Gravitational-Wave Astronomy. Oxford University Press, 2019. http://dx.doi.org/10.1093/oso/9780198568032.001.0001.

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This book provides an introduction to gravitational-wave astronomy and a survey of the physics required to understand recent breakthrough discoveries and the potential of future experiments. The material is aimed at advanced undergraduates or postgraduate students. It works as an introduction to the relevant issues and brings the reader to the level where it connects with current research. The book provides interested astronomers with an understanding of this new window to the Universe, including a relatively self-contained summary of Einstein’s geometric theory of gravity. It introduces gravitational-wave data analysts to the range of physics issues that impact on the modelling of different sources. The material also connects with fundamental physics, which is natural since gravitational-wave signals from neutron stars may help constrain our understanding of matter at extreme densities, helping nuclear and particle physicists appreciate how their models fit into the bigger picture.
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39

Neutrino Mass, Dark Matter, Gravitational Waves, Monopole Condensation, and Light Cone Quantization. Springer, 2013.

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40

Perlmutter, Arnold, Stephan L. Mintz i Behram N. Kursunogammalu. Neutrino Mass, Dark Matter, Gravitational Waves, Monopole Condensation, and Light Cone Quantization. Springer London, Limited, 2013.

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41

Braun, Arthur, Jinghua Guo, Chongmin Wang, Niels de Jonge i Rafal E. Dunin-Borkowski. In-Situ and Operando Probing of Energy Materials at Multiscale down to Single Atomic Column - The Power of X-Rays, Neutrons and Electron Microscopy. University of Cambridge ESOL Examinations, 2014.

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42

Gravity wave seeding of equatorial plasma bubbles. [Washington, DC: National Aeronautics and Space Administration, 1997.

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43

Close, Frank. 2. Nuclear alchemy. Oxford University Press, 2015. http://dx.doi.org/10.1093/actrade/9780198718635.003.0002.

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‘Nuclear alchemy’ outlines the further discoveries of protons (the carriers of positive charge in atoms) by Ernest Rutherford and neutrons (particles with no electrical charge) by James Chadwick, which led to the further explanation of atomic structure. It also describes transmutation; isotopes; gamma radioactivity; sources of radioactivity; nuclear energy scales and units; the work of Irene and Frédéric Joliot-Curie on induced radioactivity and nuclear fission; and energy waves and resolution. It was in 1932 that John Cockroft and Ernest Walton made the first nuclear particle accelerator and created a practical tool for investigating the structure of the atomic nucleus.
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44

Wang, Anzhong. Interacting Gravitational, Electromagnetic, Neutrino and Other Waves: In the Context of Einstein's General Theory of Relativity. World Scientific Publishing Co Pte Ltd, 2020.

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45

Beninger, Richard J. Life's rewards. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198824091.001.0001.

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Life’s Rewards: Linking Dopamine, Incentive Learning, Schizophrenia, and the Mind explains how increased brain dopamine produces reward-related incentive learning, the acquisition by neutral stimuli of increased ability to elicit approach and other responses. Dopamine decreases may produce inverse incentive learning, the loss by stimuli of the ability to elicit approach and other responses. Incentive learning is gradually lost when dopamine receptors are blocked. The brain has multiple memory systems defined as “declarative” and “non-declarative;” incentive learning produces one form of non-declarative memory. People with schizophrenia have hyperdopaminergia, possibly producing excessive incentive learning. Delusions may rely on declarative memory to interpret the world as it appears with excessive incentive learning. Parkinson’s disease, associated with dopamine loss, may involve a loss of incentive learning and increased inverse incentive learning. Drugs of abuse activate dopaminergic neurotransmission, leading to incentive learning about drug-associated stimuli. After withdrawal symptoms have been alleviated by detoxification treatment, drug-associated conditioned incentive stimuli will retain their ability to elicit responses until they are repeatedly experienced in the absence of primary drug rewards. Incentive learning may involve the action of dopamine at dendritic spines of striatal medium spiny neurons that have recently had glutamatergic input from assemblies of cortical neurons activated by environmental and proprioceptive stimuli. Glutamate initiates a wave of phosphorylation normally followed by a wave of phosphatase activity. If dopaminergic neurons fire, stimulation of D1 receptors prolongs the wave of phosphorylation, allowing glutamate synaptic strengthening. Activity in dopaminergic neurons in humans appears to affect mental experience.
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46

Levin, Frank S. Surfing the Quantum World. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780198808275.001.0001.

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Surfing the Quantum World bridges the gap between in-depth textbooks and typical popular science books on quantum ideas and phenomena. Among its significant features is the description of a host of mind-bending phenomena, such as a quantum object being in two places at once or a certain minus sign being the most consequential in the universe. Much of its first part is historical, starting with the ancient Greeks and their concepts of light, and ending with the creation of quantum mechanics. The second part begins by applying quantum mechanics and its probability nature to a pedagogical system, the one-dimensional box, an analog of which is a musical-instrument string. This is followed by a gentle introduction to the fundamental principles of quantum theory, whose core concepts and symbolic representations are the foundation for most of the subsequent chapters. For instance, it is shown how quantum theory explains the properties of the hydrogen atom and, via quantum spin and Pauli’s Exclusion Principle, how it accounts for the structure of the periodic table. White dwarf and neutron stars are seen to be gigantic quantum objects, while the maximum height of mountains is shown to have a quantum basis. Among the many other topics considered are a variety of interference phenomena, those that display the wave properties of particles like electrons and photons, and even of large molecules. The book concludes with a wide-ranging discussion of interpretational and philosophic issues, introduced in Chapters 14 by entanglement and 15 by Schrödinger’s cat.
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47

Armstrong, Fraser, i Katherine Blundell, red. Energy... beyond oil. Oxford University Press, 2007. http://dx.doi.org/10.1093/oso/9780199209965.001.0001.

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As the Earth's oil supply runs out, and the effects of climate change threaten nations and their populations, the search for carbon-neutral sources of energy becomes more important and increasingly urgent. This book focuses on solutions to the energy problem, and not just the problem itself. It describes the major energy-generation technologies currently under development, and provides an authoritative summary of the current status of each one. It stresses the need for a balanced portfolio of alternative energy technologies. Certain solutions will be more appropriate than others in particular locations, due to the differences in availability of natural resources such as solar, wind, wave, tidal and geothermal. In addition, nuclear options (both fission and fusion), as well as technologies such as fuel cells, photovoltaics, artificial photosynthesis and hydrogen (as an energy carrier), all have a potential role to play. A state-of-the-art critique of energy efficiency in building design is also included. Each chapter is written by an acknowledged international expert and provides a non-technical overview of the competing and complementary approaches to energy generation. Broad in scope and comprehensive in treatment, Energy..beyond Oil provides an authoritative synthesis of the scientific and technological issues which are essential to the survival of the human race in the near future. The book will be of interest and use to graduate students and researchers in all areas of energy studies, and will also be highly useful for policy-makers and professionals in the environmental sector as well as a more general readership who wish to learn more about this extremely topical subject.
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