Log in

Relevant bibliographies by topics / Dynamics of the holes / Journal articles

To see the other types of publications on this topic, follow the link: Dynamics of the holes.

Journal articles on the topic 'Dynamics of the holes'

Author: Grafiati

Published: 4 June 2021

Last updated: 1 February 2022

Create a spot-on reference in APA, MLA, Chicago, Harvard, and other styles

Select a source type:

Consult the top 50 journal articles for your research on the topic 'Dynamics of the holes.'

Next to every source in the list of references, there is an 'Add to bibliography' button. Press on it, and we will generate automatically the bibliographic reference to the chosen work in the citation style you need: APA, MLA, Harvard, Chicago, Vancouver, etc.

You can also download the full text of the academic publication as pdf and read online its abstract whenever available in the metadata.

Browse journal articles on a wide variety of disciplines and organise your bibliography correctly.

1

Hayward, Sean A. "Dynamics of Black Holes." Advanced Science Letters 2, no. 2 (2009): 205–13. http://dx.doi.org/10.1166/asl.2009.1027.

Full text

APA, Harvard, Vancouver, ISO, and other styles

2

Hemsendorf, Marc, Nils Dorband, and David Merritt. "Dynamics of supermassive black holes." Symposium - International Astronomical Union 208 (2003): 405–6. http://dx.doi.org/10.1017/s0074180900207481.

Full text

Abstract:

We are showing first results from simulations studying the effect of Brownian motion of the central mass on a cusp. N-body simulations of cuspy stellar systems around supermassive black holes represent a very challenging computational task. The wide range of dynamical timescales combined with large particle numbers required here leads us to the implementation of a systolic force calculation into a Hermite direct force block time-step scheme. With this new algorithm, we are able to handle particle numbers as large as 900000 on the parallel computers accessible to us. Due to their extraordinary

APA, Harvard, Vancouver, ISO, and other styles

3

Giddings, Steven B., and Andrew Strominger. "Dynamics of extremal black holes." Physical Review D 46, no. 2 (1992): 627–37. http://dx.doi.org/10.1103/physrevd.46.627.

Full text

APA, Harvard, Vancouver, ISO, and other styles

4

MERRITT, DAVID. "Stellar dynamics and black holes." Pramana 77, no. 1 (2011): 135–46. http://dx.doi.org/10.1007/s12043-011-0123-2.

Full text

APA, Harvard, Vancouver, ISO, and other styles

5

Andersson, Nils. "The Dynamics of Rotating Black Holes." Progress of Theoretical Physics Supplement 136 (1999): 183–98. http://dx.doi.org/10.1143/ptps.136.183.

Full text

APA, Harvard, Vancouver, ISO, and other styles

6

Inoue, Jun-ichiro, and Sadamichi Maekawa. "Dynamics of Holes in Antiferromagnetic State." Journal of the Physical Society of Japan 59, no. 6 (1990): 2110–23. http://dx.doi.org/10.1143/jpsj.59.2110.

Full text

APA, Harvard, Vancouver, ISO, and other styles

7

BRUIN, HENK, MARK DEMERS, and IAN MELBOURNE. "Existence and convergence properties of physical measures for certain dynamical systems with holes." Ergodic Theory and Dynamical Systems 30, no. 3 (2009): 687–728. http://dx.doi.org/10.1017/s0143385709000200.

Full text

Abstract:

AbstractWe study two classes of dynamical systems with holes: expanding maps of the interval and Collet–Eckmann maps with singularities. In both cases, we prove that there is a natural absolutely continuous conditionally invariant measure μ (a.c.c.i.m.) with the physical property that strictly positive Hölder continuous functions converge to the density of μ under the renormalized dynamics of the system. In addition, we construct an invariant measure ν, supported on the Cantor set of points that never escape from the system, that is ergodic and enjoys exponential decay of correlations for Höld

APA, Harvard, Vancouver, ISO, and other styles

8

Krasovsky, V. L., H. Matsumoto, and Y. Omura. "Interaction dynamics of electrostatic solitary waves." Nonlinear Processes in Geophysics 6, no. 3/4 (1999): 205–9. http://dx.doi.org/10.5194/npg-6-205-1999.

Full text

Abstract:

Abstract. Interaction of nonlinear electrostatic pulses associated with electron phase density holes moving in a collisionless plasma is studied. An elementary event of the interaction is analyzed on the basis of the energy balance in the system consisting of two electrostatic solitary waves. It is established that an intrinsic property of the system is a specific irreversibility caused by a nonadiabatic modification of the internal structure of the holes and their effective heating in the process of the interaction. This dynamical irreversibility is closely connected with phase mixing of the

APA, Harvard, Vancouver, ISO, and other styles

9

Zhang, Rui, and Yimin Zhang. "Dynamic characteristics for coal shearer cutting unit gearbox housing." Mechanics & Industry 21, no. 2 (2020): 211. http://dx.doi.org/10.1051/meca/2020008.

Full text

Abstract:

Long wall mining is most widely used in coal mining of China, and coal shearer is the most important machine due to its direct role in cutting coal. Nevertheless, coal mining enterprises are suffering from faults of coal shearer, especially cutting unit gearbox housing (CUGH). Published dynamic studies on CUGH have not considered the excitation caused by gear meshing and complete machine vibration. Due to the apparent lack of experimental validation of these published papers, the dynamic response of CUGH is not convincing. In this study, dynamic behavior of CUGH is investigated both theoretica

APA, Harvard, Vancouver, ISO, and other styles

10

NIETO, J. A., E. A. LEÓN, and V. M. VILLANUEVA. "HIGHER-DIMENSIONAL CHARGED BLACK HOLES AS CONSTRAINED SYSTEMS." International Journal of Modern Physics D 22, no. 07 (2013): 1350047. http://dx.doi.org/10.1142/s0218271813500478.

Full text

Abstract:

We construct a Lagrangian and Hamiltonian formulation for charged black holes in a d-dimensional maximally symmetric spherical space. By considering first new variables that give raise to an interesting dimensional reduction of the problem, we show that the introduction of a charge term is compatible with classical solutions to Einstein equations. In fact, we derive the well-known solutions for charged black holes, specially in the case of d = 4, where the Reissner–Nordström solution holds, without reference to Einstein field equations. We argue that our procedure may be of help for clarifying

APA, Harvard, Vancouver, ISO, and other styles

11

Fiestas, Jose A., and Rainer Spurzem. "Dynamics of Black Holes in Rotating Cores." Proceedings of the International Astronomical Union 5, S267 (2009): 328. http://dx.doi.org/10.1017/s1743921310006587.

Full text

Abstract:

We study the dynamical interaction between stars surrounding black holes in self-gravitating galaxy cores by using realistic N-body techniques, calibrated by Fokker–Planck approximated models (Fiestas, Spurzem, & Kim 2006). We study the evolution over the relaxation time (collisional nuclei) of non-spherical (triaxial) models as flattening of the system due to rotation is allowed. We follow the interplay between velocity diffusion due to relaxation and black hole star accretion and study accretion rates and cusp formation in spherically symmetric and axisymmetric models.

APA, Harvard, Vancouver, ISO, and other styles

12

Erdmenger, Johanna, Michael Haack, Matthias Kaminski, and Amos Yarom. "Fluid dynamics of R-charged black holes." Journal of High Energy Physics 2009, no. 01 (2009): 055. http://dx.doi.org/10.1088/1126-6708/2009/01/055.

Full text

APA, Harvard, Vancouver, ISO, and other styles

13

Krivan, William, Pablo Laguna, Philippos Papadopoulos, and Nils Andersson. "Dynamics of perturbations of rotating black holes." Physical Review D 56, no. 6 (1997): 3395–404. http://dx.doi.org/10.1103/physrevd.56.3395.

Full text

APA, Harvard, Vancouver, ISO, and other styles

14

Gutowski, J., and G. Papadopoulos. "The dynamics of very special black holes." Physics Letters B 472, no. 1-2 (2000): 45–53. http://dx.doi.org/10.1016/s0370-2693(99)01412-4.

Full text

APA, Harvard, Vancouver, ISO, and other styles

15

Inoue, Jun-ichiro, and Sadamichi Maekawa. "Dynamics of Two Holes in thet-JModel." Progress of Theoretical Physics Supplement 108 (1992): 313–26. http://dx.doi.org/10.1143/ptps.108.313.

Full text

APA, Harvard, Vancouver, ISO, and other styles

16

Meunier, N. "Large-scale photospheric dynamics below coronal holes." Astronomy & Astrophysics 443, no. 1 (2005): 309–17. http://dx.doi.org/10.1051/0004-6361:20053249.

Full text

APA, Harvard, Vancouver, ISO, and other styles

17

Till, Rainer, and Fritz Keilmann. "Dynamics of low-energy holes in germanium." Physical Review B 44, no. 4 (1991): 1554–64. http://dx.doi.org/10.1103/physrevb.44.1554.

Full text

APA, Harvard, Vancouver, ISO, and other styles

18

Lopes Filho, Milton da Costa, and Helena J. Nussenzveig Lopes. "Vortex dynamics on a domain with holes." Theoretical and Computational Fluid Dynamics 24, no. 1-4 (2009): 51–57. http://dx.doi.org/10.1007/s00162-009-0141-6.

Full text

APA, Harvard, Vancouver, ISO, and other styles

19

Chulkov, E. V., A. Leonardo, I. Yu Sklyadneva, and V. M. Silkin. "Dynamics of electrons and holes at surfaces." Applied Surface Science 254, no. 1 (2007): 383–86. http://dx.doi.org/10.1016/j.apsusc.2007.07.050.

Full text

APA, Harvard, Vancouver, ISO, and other styles

20

Zhang, Baocheng. "Thermodynamics of Acoustic Black Holes in Two Dimensions." Advances in High Energy Physics 2016 (2016): 1–8. http://dx.doi.org/10.1155/2016/5710625.

Full text

Abstract:

It is well-known that the thermal Hawking-like radiation can be emitted from the acoustic horizon, but the thermodynamic-like understanding for acoustic black holes was rarely made. In this paper, we will show that the kinematic connection can lead to the dynamic connection at the horizon between the fluid and gravitational models in two dimensions, which implies that there exists the thermodynamic-like description for acoustic black holes. Then, we discuss the first law of thermodynamics for the acoustic black hole via an intriguing connection between the gravitational-like dynamics of the ac

APA, Harvard, Vancouver, ISO, and other styles

21

Eliasson, B., and P. K. Shukla. "The dynamics of electron and ion holes in a collisionless plasma." Nonlinear Processes in Geophysics 12, no. 2 (2005): 269–89. http://dx.doi.org/10.5194/npg-12-269-2005.

Full text

Abstract:

Abstract. We present a review of recent analytical and numerical studies of the dynamics of electron and ion holes in a collisionless plasma. The new results are based on the class of analytic solutions which were found by Schamel more than three decades ago, and which here work as initial conditions to numerical simulations of the dynamics of ion and electron holes and their interaction with radiation and the background plasma. Our analytic and numerical studies reveal that ion holes in an electron-ion plasma can trap Langmuir waves, due the local electron density depletion associated with th

APA, Harvard, Vancouver, ISO, and other styles

22

Levine, Robyn. "Large Dynamic Range Simulations of Galaxies Hosting Supermassive Black Holes." Proceedings of the International Astronomical Union 6, S271 (2010): 153–59. http://dx.doi.org/10.1017/s174392131101756x.

Full text

Abstract:

AbstractThe co-evolution of supermassive black holes (SMBHs) and their host galaxies is a rich problem, spanning a large-dynamic range and depending on many physical processes. Simulating the transport of gas and angular momentum from super-galactic scales all the way down to the outer edge of the black hole's accretion disk requires sophisticated numerical techniques with extensive treatment of baryonic physics. We use a hydrodynamic adaptive mesh refinement simulation to follow the growth and evolution of a typical disk galaxy hosting an SMBH, in a cosmological context (covering a dynamical

APA, Harvard, Vancouver, ISO, and other styles

23

Clausen, Sigmund, Geir Helgensen, and Arne T. Skjeltorp. "Braid Description of Few Body Dynamics." International Journal of Bifurcation and Chaos 08, no. 07 (1998): 1383–97. http://dx.doi.org/10.1142/s021812749800108x.

Full text

Abstract:

A few body system of magnetic holes set in motion by external ac magnetic fields is studied both experimentally and numerically. Notions from braid theory are used to describe the dynamics ina very compact manner. The time histroy of n magnetic holes moving in a plane is represented by an n-strand braid which enables us to extrat periodic orbits and to map out phase phase portraits. The transitions between different periodic modes of motion are either continuous or noncontinuous followed by strong hysteresis.

APA, Harvard, Vancouver, ISO, and other styles

24

Sridhar, S., and J. Touma. "Stellar dynamics around black holes in galactic nuclei." Monthly Notices of the Royal Astronomical Society 303, no. 3 (1999): 483–94. http://dx.doi.org/10.1046/j.1365-8711.1999.02218.x.

Full text

APA, Harvard, Vancouver, ISO, and other styles

25

CHOWDHURY, BORUN D. "BLACK HOLES VERSUS FIREWALLS AND THERMO-FIELD DYNAMICS." International Journal of Modern Physics D 22, no. 12 (2013): 1342011. http://dx.doi.org/10.1142/s021827181342011x.

Full text

Abstract:

In this paper, we examine the implications of the ongoing black holes versus firewalls debate for the thermo-field dynamics of black holes by analyzing a conformal field theory (CFT) in a thermal state in the context of anti-de Sitter/CFT. We argue that the thermo-field doubled copy of the thermal CFT should be thought of not as a fictitious system, but as the image of the CFT in the heat bath. In case of strong coupling between the CFT and the heat bath, this image allows for free infall through the horizon and the system is described by a black hole. Conversely, firewalls are the appropriate

APA, Harvard, Vancouver, ISO, and other styles

26

Maldacena, Juan, and Andrew Strominger. "Universal low-energy dynamics for rotating black holes." Physical Review D 56, no. 8 (1997): 4975–83. http://dx.doi.org/10.1103/physrevd.56.4975.

Full text

APA, Harvard, Vancouver, ISO, and other styles

27

Chicone, C., and B. Mashhoon. "Tidal dynamics of relativistic flows near black holes." Annalen der Physik 14, no. 5 (2005): 290–308. http://dx.doi.org/10.1002/andp.200410126.

Full text

APA, Harvard, Vancouver, ISO, and other styles

28

Wang, Lidong, Michal Bledowski, Ayyappan Ramakrishnan, and Radim Beranek. "TiO2-Polyheptazine Hybrid Photoelectrodes: Dynamics of Photogenerated Holes." ECS Transactions 35, no. 25 (2019): 173–82. http://dx.doi.org/10.1149/1.3655523.

Full text

APA, Harvard, Vancouver, ISO, and other styles

29

INOUE, J., and S. MAEKAWA. "DYNAMICS OF HOLES IN THE Cu-OXIDE SUPERCONDUCTORS." Modern Physics Letters B 03, no. 16 (1989): 1191–95. http://dx.doi.org/10.1142/s0217984989001825.

Full text

APA, Harvard, Vancouver, ISO, and other styles

30

Shustov, Pavel I., Ilya V. Kuzichev, Ivan Y. Vasko, Anton V. Artemyev, and Andrew J. Gerrard. "The dynamics of electron holes in current sheets." Physics of Plasmas 28, no. 1 (2021): 012902. http://dx.doi.org/10.1063/5.0029999.

Full text

APA, Harvard, Vancouver, ISO, and other styles

31

Merritt, David. "Dynamics of galaxy cores and supermassive black holes." Reports on Progress in Physics 69, no. 9 (2006): 2513–79. http://dx.doi.org/10.1088/0034-4885/69/9/r01.

Full text

APA, Harvard, Vancouver, ISO, and other styles

32

Ribeiro Junior, Luiz Antonio, and Wiliam Ferreira da Cunha. "Nonadiabatic dynamics of injected holes in conjugated polymers." Physical Chemistry Chemical Physics 19, no. 15 (2017): 10000–10008. http://dx.doi.org/10.1039/c7cp00729a.

Full text

Abstract:

The dynamics of injected holes in short transient times that precede polaron formation is numerically studied in the framework of a tight-binding electron–phonon interacting approach aimed at describing organic one-dimensional lattices.

APA, Harvard, Vancouver, ISO, and other styles

33

Sherman, A. V. "Dynamics of holes in the extended Hubbard model." Physical Review B 46, no. 10 (1992): 6400–6408. http://dx.doi.org/10.1103/physrevb.46.6400.

Full text

APA, Harvard, Vancouver, ISO, and other styles

34

Volonteri, Marta, Tamara Bogdanović, Massimo Dotti, and Monica Colpi. "Massive Black Holes in Merging Galaxies." Proceedings of the International Astronomical Union 11, A29B (2015): 285–91. http://dx.doi.org/10.1017/s1743921316005366.

Full text

Abstract:

AbstractThe dynamics of massive black holes (BHs) in galaxy mergers is a rich field of research that has seen much progress in recent years. In this contribution we briefly review the processes describing the journey of BHs during mergers, from the cosmic context all the way to when BHs coalesce. If two galaxies each hosting a central BH merge, the BHs would be dragged towards the center of the newly formed galaxy. If/when the holes get sufficiently close, they coalesce via the emission of gravitational waves. How often two BHs are involved in galaxy mergers depends crucially on how many galax

APA, Harvard, Vancouver, ISO, and other styles

35

Prihadi, Hadyan L., Muhammad F. A. R. Sakti, Getbogi Hikmawan, and Freddy P. Zen. "Dynamics of charged and rotating NUT black holes in Rastall gravity." International Journal of Modern Physics D 29, no. 03 (2020): 2050021. http://dx.doi.org/10.1142/s0218271820500212.

Full text

Abstract:

In this work, the Kerr–Newman-NUT black hole solution in Rastall gravity is proposed and it turns out that the horizon is [Formula: see text] dependence. Black hole dynamics such as the event horizons, ergosurface, zero angular momentum observer (ZAMO), thermodynamic properties, and the equatorial circular orbit around the black hole such as static radius limit, null equatorial circular orbit, and innermost stable circular orbit are investigated in this work. How the NUT and Rastall parameter affect the dynamic of the black hole is also shown.

APA, Harvard, Vancouver, ISO, and other styles

36

Dandekar, Yogesh. "Membrane-gravity correspondence." International Journal of Modern Physics D 28, no. 14 (2019): 1944014. http://dx.doi.org/10.1142/s0218271819440140.

Full text

Abstract:

We discuss a novel description of the dynamics of black holes in terms of the dynamics of “Membranes”. The membrane description emerges naturally if we consider black holes in the limit of a large number of spacetime dimensions [Formula: see text]. This “Large [Formula: see text] membrane paradigm” can be systematically constructed in a perturbation theory in [Formula: see text]. A similar membrane description can be constructed for the case of finite-dimensional black holes — and it reproduces black hole dynamics correctly in some nontrivial cases — which is quite striking.

APA, Harvard, Vancouver, ISO, and other styles

37

Narzilloev, Bakhtiyor, Javlon Rayimbaev, Ahmadjon Abdujabbarov, and Bobomurat Ahmedov. "Regular Bardeen Black Holes in Anti-de Sitter Spacetime versus Kerr Black Holes through Particle Dynamics." Galaxies 9, no. 3 (2021): 63. http://dx.doi.org/10.3390/galaxies9030063.

Full text

Abstract:

In this work, test particle dynamics around a static regular Bardeen black hole (BH) in Anti-de Sitter spacetime has been studied. It has been shown for neutral test particles that parameters of a regular Bardeen black hole in Anti-de Sitter spacetime can mimic the rotation parameter of the Kerr metric up to the value a≈0.9 providing the same innermost stable circular orbit (ISCO) radius. We have also explored the dynamics of magnetized particles with a magnetic dipole moment around a magnetically charged regular Bardeen black hole in Anti-de Sitter spacetime. As a realistic astrophysical scen

APA, Harvard, Vancouver, ISO, and other styles

38

Han, W. B. "Dynamics of particles in slowly rotating black holes with dipolar halos." Proceedings of the International Astronomical Union 3, S248 (2007): 498–99. http://dx.doi.org/10.1017/s1743921308019935.

Full text

Abstract:

AbstractIn general, the model of galaxy assumes a central huge black hole surrounded by a massive halo, disk or ring. In this paper, we investigate the gravitational field structure of a slowly rotating black hole with a dipolar halo, and the dynamics and chaos of test particles moving in it. Using Poincaré sections and fast Lyapunov indicator (FLI) in general relativity, we investigate chaos under different dynamical parameters, and find that the FLI is suitable for detecting chaos and even resonant orbits.

APA, Harvard, Vancouver, ISO, and other styles

39

Freitag, Marc, James E. Dale, Ross P. Church, and Melvyn B. Davies. "Dynamics of galactic nuclei: mass segregation and collisions." Proceedings of the International Astronomical Union 3, S245 (2007): 211–14. http://dx.doi.org/10.1017/s1743921308017675.

Full text

Abstract:

AbstractMassive black holes (MBHs) with a mass below ~ 107 M⊙ are likely to reside at the centre of dense stellar nuclei shaped by 2-body relaxation, close interactions with the MBH and direct collisions. In this contribution, we stress the role of mass segregation of stellar-mass black holes into the innermost tenths of a parsec and point to the importance of hydrodynamical collisions between stars. At the Galactic centre, collisions must affect giant stars and some of the S-stars.

APA, Harvard, Vancouver, ISO, and other styles

40

Binney, James. "Symposium summary: dynamics." Proceedings of the International Astronomical Union 3, S245 (2007): 455–58. http://dx.doi.org/10.1017/s1743921308018358.

Full text

Abstract:

AbstractPseudobulges form from unstable disks, while classical bulges form in violent episodes of star formation when a merger sweeps cold gas to a galactic centre. It seems unlikely that smashed disks contribute much to classical bulges. During mergers central black holes make cusps shallower and inflate kinematically decoupled cores. The abundance of galaxies with no detected classical bulge can perhaps be understood if galaxies exchange gas with the IGM more freely than is often supposed.

APA, Harvard, Vancouver, ISO, and other styles

41

Zang, Jinjuan, and Haibin Yang. "The Dynamics of Structural Holes: Status and Technology Asymmetry." Academy of Management Proceedings 2016, no. 1 (2016): 16554. http://dx.doi.org/10.5465/ambpp.2016.16554abstract.

Full text

APA, Harvard, Vancouver, ISO, and other styles

42

Takeda, Tsuyoshi, and Keiichiro Yamagiwa. "Dynamics of electron-beam holes induced by self-trapping." Physics Letters A 339, no. 1-2 (2005): 118–22. http://dx.doi.org/10.1016/j.physleta.2005.03.016.

Full text

APA, Harvard, Vancouver, ISO, and other styles

43

BUNDFUSS, STEFAN, TYLL KRÜGER, and SERGE TROUBETZKOY. "Topological and symbolic dynamics for hyperbolic systems with holes." Ergodic Theory and Dynamical Systems 31, no. 5 (2010): 1305–23. http://dx.doi.org/10.1017/s0143385710000556.

Full text

Abstract:

AbstractWe consider an axiom A diffeomorphism or a Markov map of an interval and the invariant set Ω* of orbits which never falls into a fixed hole. We study various aspects of the symbolic representation of Ω* and of its non-wandering set Ωnw. Our results are on the cardinality of the set of topologically transitive components of Ωnw and their structure. We also prove that Ω* is generically a subshift of finite type in several senses.

APA, Harvard, Vancouver, ISO, and other styles

44

Thorne, K. S. "Classical Black Holes: The Nonlinear Dynamics of Curved Spacetime." Science 337, no. 6094 (2012): 536–38. http://dx.doi.org/10.1126/science.1225474.

Full text

APA, Harvard, Vancouver, ISO, and other styles

45

Gambini, Rodolfo, Javier Olmedo, and Jorge Pullin. "Schrödinger-like quantum dynamics in loop quantized black holes." International Journal of Modern Physics D 25, no. 08 (2016): 1642006. http://dx.doi.org/10.1142/s0218271816420062.

Full text

Abstract:

We show, following a previous quantization of a vacuum spherically symmetric spacetime carried out in [R. Gambini, J. Olmedo and J. Pullin, Class. Quantum Grav. 31 (2014) 095009.] that this setting admits a Schrödinger-like picture. More precisely, the technique adopted there for the definition of parametrized Dirac observables (that codify local information of the quantum theory) can be extended in order to accommodate different pictures. In this new picture, the quantum states are parametrized in terms of suitable gauge parameters and the observables constructed out of the kinematical ones o

APA, Harvard, Vancouver, ISO, and other styles

46

Zanotti, Olindo, José A. Font, Luciano Rezzolla, and Pedro J. Montero. "Dynamics of oscillating relativistic tori around Kerr black holes." Monthly Notices of the Royal Astronomical Society 356, no. 4 (2005): 1371–82. http://dx.doi.org/10.1111/j.1365-2966.2004.08567.x.

Full text

APA, Harvard, Vancouver, ISO, and other styles

47

Khuri, Ramzi R., and Robert C. Myers. "Dynamics of extreme black holes and massive string states." Physical Review D 52, no. 12 (1995): 6988–96. http://dx.doi.org/10.1103/physrevd.52.6988.

Full text

APA, Harvard, Vancouver, ISO, and other styles

48

Khromykh, Leonid A., and Alexander A. Kirillov. "The gravitational dynamics of the primordial black holes cluster." Journal of Physics: Conference Series 1390 (November 2019): 012090. http://dx.doi.org/10.1088/1742-6596/1390/1/012090.

Full text

APA, Harvard, Vancouver, ISO, and other styles

49

Barrabaes, C., B. Boisseau, and W. Israel. "Orbits, forces and accretion dynamics near spinning black holes." Monthly Notices of the Royal Astronomical Society 276, no. 2 (1995): 432–38. http://dx.doi.org/10.1093/mnras/276.2.432.

Full text

APA, Harvard, Vancouver, ISO, and other styles

50

Ponce, Marcelo, Joshua A. Faber, and James C. Lombardi. "ACCRETION DISKS AROUND KICKED BLACK HOLES: POST-KICK DYNAMICS." Astrophysical Journal 745, no. 1 (2011): 71. http://dx.doi.org/10.1088/0004-637x/745/1/71.

Full text

APA, Harvard, Vancouver, ISO, and other styles

We offer discounts on all premium plans for authors whose works are included in thematic literature selections. Contact us to get a unique promo code!