標(biāo)題: Titlebook: 2nd Karl Schwarzschild Meeting on Gravitational Physics; Piero Nicolini,Matthias Kaminski,Marcus Bleicher Conference proceedings 2018 Spri [打印本頁] 作者: TEMPO 時(shí)間: 2025-3-21 19:03
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書目名稱2nd Karl Schwarzschild Meeting on Gravitational Physics年度引用學(xué)科排名
書目名稱2nd Karl Schwarzschild Meeting on Gravitational Physics讀者反饋
書目名稱2nd Karl Schwarzschild Meeting on Gravitational Physics讀者反饋學(xué)科排名
作者: Antagonism 時(shí)間: 2025-3-22 00:14
Samuel Hahnemann: Rebarbative Genius,pproach is general and may be applied for several cases of interest. We also show that our treatment is compatible with the standard approach of general relativity, evaluating the motion of a freely falling particle in the context of our metric.作者: ROOF 時(shí)間: 2025-3-22 01:10
Basavaprabhu L. Patil,P. Lava Kumarransition similar to the liquid/gas transition of a real fluid. In the present analysis, we have considered the cosmological constant as a dynamical quantity, and its variation is included in the first law of black hole thermodynamics.作者: 跟隨 時(shí)間: 2025-3-22 07:25
Conference proceedings 2018y and information..Specialists in the field of black hole physics and rising young researchers present the latest findings on the broad topic of black holes, gravity, and information, highlighting its applications to astrophysics, cosmology, particle physics, and strongly correlated systems..作者: 喊叫 時(shí)間: 2025-3-22 09:13 作者: 控訴 時(shí)間: 2025-3-22 14:25 作者: 常到 時(shí)間: 2025-3-22 20:15 作者: 舊病復(fù)發(fā) 時(shí)間: 2025-3-22 22:26 作者: 雜色 時(shí)間: 2025-3-23 04:21
,An Historical Overview, 1900–1949,ating the charge on the rotating charged AdS black hole background constructed by the fluid/gravity derivative expansion, we show that the Chern–Simons contribution to black hole entropy agrees with the anomaly-induced entropy current in the dual conformal field theory at the leading order of the derivative expansion.作者: 大酒杯 時(shí)間: 2025-3-23 06:51 作者: Melodrama 時(shí)間: 2025-3-23 12:40
How Are Sovereign Ratings Assigned?,e corrections to the standard General Relativistic predictions for the perihelion precession for planets in the solar system. This analysis allows us to set bounds for the GUP deformation parameter from well-known astronomical measurements.作者: 符合國情 時(shí)間: 2025-3-23 15:41
https://doi.org/10.1007/978-3-319-57156-0ts on the small distance behaviour. It is not known whether theories can be constructed that obey these constraints; if so, all interaction parameters that are normally freely adjustable, would become computable.作者: FLIRT 時(shí)間: 2025-3-23 18:37
Claire A. Amuhaya,Denis A. Degterev) theory, and restrict our attention to four-dimensional, static, non-rotating black holes for simplicity. We outline some of the menagerie of EYM solutions in both asymptotically flat and asymptotically anti-de Sitter space. We attempt to make sense of this black hole zoo in terms of Bizon’s modified no-hair conjecture.作者: 外形 時(shí)間: 2025-3-23 22:58
https://doi.org/10.1007/978-3-319-94256-8Black Hole Theory; Karl Schwarzschild; Black Hole Evaporation; Black Hole Thermodynamics; Black Hole Hol作者: 一大塊 時(shí)間: 2025-3-24 04:57
978-3-030-06821-9Springer Nature Switzerland AG 2018作者: FILLY 時(shí)間: 2025-3-24 09:15
Piero Nicolini,Matthias Kaminski,Marcus BleicherCovers a broad range of black hole physics.With contributions of leading experts in the field.Including a panel discussion with the Nobel laureate Gerard ‘t Hooft and other leading experts in the fiel作者: 干旱 時(shí)間: 2025-3-24 12:43 作者: Morphine 時(shí)間: 2025-3-24 18:41 作者: Colonoscopy 時(shí)間: 2025-3-24 21:50
A Century of Monetary Policy at the FedTheoretical physicists are all agreed that Semiclassical Black holes are paradoxical objects (as nicely reconfirmed by several discussions during the Karl Schwarzschild meeting 2015). However, a clear strategy in order to solve this problem is still unknown.作者: filicide 時(shí)間: 2025-3-25 01:57 作者: instulate 時(shí)間: 2025-3-25 03:20
https://doi.org/10.1007/978-3-319-57156-0re. The conformal component of the metric field is then treated as a dilaton field with only renormalizable interactions. This imposes constraints on the theory, which can also be viewed as demanding regularity of the action as the dilaton field variable tends to 0. In other words, we have constrain作者: 柱廊 時(shí)間: 2025-3-25 11:22
Theory III: Interstate Conflicts,tion and black holes, and how to effectively treat quantization of the background spacetime. Modern perspectives on black hole evaporation suggest that quantum gravity effects in the near-horizon region can perturb the local geometry. The approaches differ, however, in the time scale on which one ca作者: 健談 時(shí)間: 2025-3-25 13:04 作者: 比目魚 時(shí)間: 2025-3-25 15:51
RESEARCH IN FLUID MECHANICS: FLOWS, Near the singularity the black hole behaves as the Janis-Newmann-Winicour-Wyman solution. The hairy black hole solutions allow for consistent thermodynamical description. At large mass they have the same thermodynamical behaviour of the Schwarzschild black hole, whereas for small masses they differ作者: 翻布尋找 時(shí)間: 2025-3-25 22:56
Samuel Hahnemann: Rebarbative Genius,alidity of a complex coordinate transformation, which acts on the spherically symmetric metric and permits one to infer the corresponding .(.) modification. The consequences of this recipe are here described, giving particular emphasis to define a class of compatible axially symmetric solutions, whi作者: Compatriot 時(shí)間: 2025-3-26 01:24
Samuel Hahnemann: Rebarbative Genius,mmetries of this phase space and compute their corresponding conserved charges. We show that the symmetry algebra is an interesting generalization of Virasoro algebra. The analysis is based on covariant phase space method.作者: hazard 時(shí)間: 2025-3-26 04:41
Bubbles, Foams and Other Fragile Objects,this instability. We find hairy black hole solutions of a fully coupled system of Einstein gravity and a charged scalar field. The black holes are surrounded by a reflecting mirror. We also investigate the stability of these black holes.作者: 同來核對 時(shí)間: 2025-3-26 10:18
https://doi.org/10.1007/978-3-031-54964-9 background provided by Schwarzschild’s solution. The reason is that this solution has singularities, widely regarded as a big problem of GR. While the event horizon singularity can be removed by moving to non-singular coordinates, not the same is true about the . singularity. However, I will presen作者: 障礙物 時(shí)間: 2025-3-26 15:35 作者: compel 時(shí)間: 2025-3-26 20:39
Saying Oops after Assuming the Chairmanshipg limit to the class of Kerr-AdS metrics, and have a number of intriguing properties. Their event horizons are not compact but have finite area, they have no closed timelike curves, and their entropy is larger than expected from general considerations of their thermodynamic volume. Here a brief over作者: 改良 時(shí)間: 2025-3-26 21:17 作者: 改變 時(shí)間: 2025-3-27 01:41 作者: 流出 時(shí)間: 2025-3-27 08:52 作者: BATE 時(shí)間: 2025-3-27 11:34
,Clement Attlee — Quiet Revolutionary,d to improve the short distance behaviour of classical black hole spacetimes by invoking nonlocal modifications of the gravity action. We present the problem of extending such a GUP scenario to higher dimensional spacetimes and we critically review the existing literature on the topic.作者: 反話 時(shí)間: 2025-3-27 14:02 作者: Introvert 時(shí)間: 2025-3-27 18:39 作者: exceed 時(shí)間: 2025-3-28 01:35
RESEARCH IN FLUID MECHANICS: FLOWS, Near the singularity the black hole behaves as the Janis-Newmann-Winicour-Wyman solution. The hairy black hole solutions allow for consistent thermodynamical description. At large mass they have the same thermodynamical behaviour of the Schwarzschild black hole, whereas for small masses they differ substantially from the latter.作者: 不透明 時(shí)間: 2025-3-28 05:06 作者: Metastasis 時(shí)間: 2025-3-28 08:42 作者: Injunction 時(shí)間: 2025-3-28 13:37
,Clement Attlee — Quiet Revolutionary,d to improve the short distance behaviour of classical black hole spacetimes by invoking nonlocal modifications of the gravity action. We present the problem of extending such a GUP scenario to higher dimensional spacetimes and we critically review the existing literature on the topic.作者: formula 時(shí)間: 2025-3-28 14:54 作者: insert 時(shí)間: 2025-3-28 21:25 作者: 前兆 時(shí)間: 2025-3-29 01:59
Singularities, Horizons, Firewalls, and Local Conformal Symmetry,ansion of a stent can occur and covered stents are now electively placed in very tight stenoses. They are also able to seal aneurysms or dissections from previous surgery, balloon dilation or bare-metal stents. Open-cell stents allow access to side branches “jailed” by the stent and dilating and ste作者: Chagrin 時(shí)間: 2025-3-29 06:35
,Panel Discussion, “The Duel”: The Good, the Bad, and the Ugly of Gravity and Information,ield stimulation) demonstrated that contracting cells decreased from 60 to 2%. Contractile amplitude (percent shortening) decreases significantly from 5.6 vs. 2.4% with no change in time to peak twitch. Recombinant adenovirus overexpressing mutated β2 subunits in adult mammalian myocytes can markedl作者: 自作多情 時(shí)間: 2025-3-29 11:15 作者: 相信 時(shí)間: 2025-3-29 12:54 作者: 值得尊敬 時(shí)間: 2025-3-29 19:06 作者: 有機(jī)體 時(shí)間: 2025-3-29 20:51
Symplectic Structure of Extremal Black Holeshat predispose to both systolic and diastolic disorders. The importance of hypertension, anemia, hyperparathyroidism, hyper- lipidemia, and diabetes mellitus in predisposing to these abnormalities is reviewed splendidly by researchers active in these areas. The final section concentrates on therapeutics. Data978-1-4613-6741-3978-1-4615-3902-5作者: Barter 時(shí)間: 2025-3-30 03:40 作者: ALTER 時(shí)間: 2025-3-30 06:26 作者: saphenous-vein 時(shí)間: 2025-3-30 11:46 作者: Aggregate 時(shí)間: 2025-3-30 12:23
Aspects of Quantum Chaos Inside Black Holest venipuncture sites..Echocardiography is paramount to evaluating IE. Two-dimensional imaging can detect vegetations as small as 2 mm. Transthoracic echocardiography is adequate for initial rapid imaging. Transesophageal echocardiography can be more useful in evaluating patients with complex congeni作者: 吞下 時(shí)間: 2025-3-30 16:55
Black Hole Entropy in the Presence of Chern–Simons Term and Holographyardial transformation did not significantly reduce myocardial performance and pumping ability, but caused a decrease in oxygen consumption as related to developed stress and LV weight. Thus, the efficiency of the hypertrophied ventricle of SHR was improved. However, due to the moderate effect of iso作者: adjacent 時(shí)間: 2025-3-30 23:44 作者: STALE 時(shí)間: 2025-3-31 02:40 作者: Arboreal 時(shí)間: 2025-3-31 05:05 作者: blackout 時(shí)間: 2025-3-31 09:46 作者: hair-bulb 時(shí)間: 2025-3-31 15:54
2nd Karl Schwarzschild Meeting on Gravitational Physics作者: STELL 時(shí)間: 2025-3-31 20:01
The Good Properties of Schwarzschild’s Singularitye encountered and summarizing the important learning objectives in a succinct way. Covering clinical electrophysiology, device troubleshooting and analysis as well as intracardiac electrogram analysis and ablat978-3-030-28533-3作者: Apogee 時(shí)間: 2025-4-1 00:43
