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A study of the infrared emission of SGR/AXPs in a disk scenario and its implications for their origin 盘状场景下SGR/ axp红外发射的研究及其对其起源的影响
Pub Date : 2023-01-24 DOI: 10.1142/9789811269776_0381
Sarah V. Borges
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引用次数: 0
Dark matter as condensed phase of generic bosons 暗物质是一般玻色子的凝聚相
Pub Date : 2023-01-24 DOI: 10.1142/9789811269776_0120
E. Castellanos, Jorge Mastache
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引用次数: 0
The passage of time and top-down causation 时间的流逝和自上而下的因果关系
Pub Date : 2023-01-24 DOI: 10.1142/9789811269776_0300
B. Drossel
It is often claimed that the fundamental laws of physics are deterministic and time-symmetric and that therefore our experience of the passage of time is an illusion. This paper will critically discuss these claims and show that they are based on the misconception that the laws of physics are an exact and complete description of nature. I will argue that all supposedly fundamental deterministic and time-symmetric laws have their limitations and are supplemented by stochastic and irreversible elements. In fact, a deterministic description of a system is valid only as long as interactions with the rest of the world can be ignored. The most famous example is the quantum measurement process that occurs when a quantum system interacts with a macroscopic environment such as a measurement apparatus. This environment determines in a top-down way the possible outcomes of the measurement and their probabilities. I will argue that more generally the possible events that can occur in a system and their probabilities are the result of top-down influences from the wider context. In this way the microscopic level of a system is causally open to influences from the macroscopic environment. In conclusion, indeterminism and irreversibility are the result of a system being embedded in a wider context.
人们经常声称,物理的基本定律是决定性的,是时间对称的,因此我们对时间流逝的体验是一种错觉。本文将批判性地讨论这些说法,并表明它们是基于物理定律是对自然的精确和完整描述的误解。我认为,所有被认为是基本的确定性和时间对称定律都有其局限性,并辅以随机和不可逆的因素。事实上,只有当与世界其他部分的交互可以被忽略时,系统的确定性描述才是有效的。最著名的例子是当量子系统与宏观环境(如测量仪器)相互作用时发生的量子测量过程。这种环境以一种自上而下的方式决定了测量的可能结果及其概率。我认为,更一般地说,系统中可能发生的事件及其概率是来自更广泛背景的自上而下影响的结果。这样,系统的微观层面就会受到宏观环境的影响。总之,不确定性和不可逆性是一个系统被嵌入一个更广泛的背景的结果。
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引用次数: 2
Explaining time’s passage 解释时间的流逝
Pub Date : 2023-01-24 DOI: 10.1142/9789811269776_0301
J. Dickau
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引用次数: 0
Kilonova emission observed so far: A comparison with AT2017gfo 迄今为止观测到的千新星辐射:与AT2017gfo的比较
Pub Date : 2023-01-24 DOI: 10.1142/9789811269776_0259
A. Rossi
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引用次数: 0
Theoretical implications on the very high energy emission from GRB 190114C GRB 190114C高能辐射的理论意义
Pub Date : 2023-01-24 DOI: 10.1142/9789811269776_0247
D. Miceli, A. Berti, Ž. Bošnjak, S. Covino, S. Fukami, S. Inoue, F. Longo, R. Mirzoyan, E. Moretti, L. Nava, K. Noda, D. Paneque, A. Stamerra, Y. Suda, I. Vovk
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引用次数: 0
Reconstruction of a star motion in the vicinity of black hole from the redshift of the electromagnetic spectrum 从电磁波谱的红移重建黑洞附近的恒星运动
Pub Date : 2023-01-24 DOI: 10.1142/9789811269776_0092
S. Komarov, A. Gorbatsievich
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引用次数: 0
Searching for Gamma-Ray Bursts with the High-Altitude Water Cherenkov (HAWC) observatory 用高海拔水切伦科夫(HAWC)天文台寻找伽马射线暴
Pub Date : 2023-01-24 DOI: 10.1142/9789811269776_0249
K. Engel
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引用次数: 0
MASTER optical observations of the blazar TXS0506+056 during the IC170922A IC170922A期间blazar TXS0506+056的主光学观测
Pub Date : 2023-01-24 DOI: 10.1142/9789811269776_0117
V. Lipunov, K. Zhirkov, V. Kornilov, E. Gorbovskoy, N. Budnev, D. Buckley, R. Rebolo, M. Serra, R. Podesta, C. Francile, V. Topolev, N. Tiurina, O. Gress, P. Balanutsa, A. Chasovnikov, D. Vlasenko, E. Minkina, A. Gabovich, G. Antipov, A. Kuznetsov, V. Vladimirov, S. Svertilov, F. Podestà, V. Grinshpun, A. Tlatov, D. Cheryasov, V. Senik
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引用次数: 0
Conformal dilaton gravity, antipodal mapping and black hole physics on a warped spacetime 翘曲时空中的共形膨胀、重力、对映映射和黑洞物理
Pub Date : 2023-01-24 DOI: 10.1142/9789811269776_0076
R. J. Slagter
An exact time-dependent solution of a black hole is found in a conformally invariant gravity model on a warped Randall-Sundrum spacetime, by writing the metric gμν = ω 4 n−2 g̃μν . Here g̃μν represents the ”un-physical” spacetime and ω the dilaton field, which will be treated on equal footing as any renormalizable scalar field. It is remarkable that the 5D and 4D effective field equations for the metric components and dilaton fields can be written in general dimension n = 4, 5. The location of the horizon(s) are determined by a quintic polynomial. This polynomial is related to the symmetry group of the icosahedron, isomorphic with the Galois group A5. We applied the antipodal mapping on the axially symmetric black hole spacetime and make some connection with the information and firewall paradoxes. The dilaton field can be used to describe the different notion the in-going and outside observers have of the Hawking radiation by using different conformal gauge freedom. The disagreement about the interior of the black hole is explained by the antipodal map of points on the horizon. The free parameters of the solution can be chosen in such a way that ḡμν is singular-free and topologically regular, even for ω → 0.
在弯曲Randall-Sundrum时空上的共形不变引力模型中,通过度量gμν = ω 4 n−2 gμν,找到了黑洞的精确时变解。这里g μν表示“非物理的”时空,ω表示膨胀场,它将被视为任何可重整的标量场。值得注意的是,度量分量和膨胀场的5D和4D有效场方程可以写成一般维数n = 4,5。视界的位置由一个五次多项式确定。该多项式与二十面体对称群有关,与伽罗瓦群A5同构。将对映映射应用于轴对称黑洞时空,并与信息悖论和防火墙悖论联系起来。膨胀场可以通过使用不同的共形规范自由度来描述进入和外部观察者对霍金辐射的不同概念。关于黑洞内部的分歧可以用视界上点的对映图来解释。该解的自由参数可以这样选择:即使ω→0,ḡμν也是无奇异且拓扑正则的。
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引用次数: 0
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The Sixteenth Marcel Grossmann Meeting
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