標(biāo)題: Titlebook: Neutron Stars 1; Equation of State an P. Haensel,A. Y. Potekhin,D. G. Yakovlev Textbook 2007 Springer-Verlag New York 2007 Star.Universe.bo [打印本頁(yè)] 作者: dejected 時(shí)間: 2025-3-21 17:56
書(shū)目名稱(chēng)Neutron Stars 1影響因子(影響力)
作者: Goblet-Cells 時(shí)間: 2025-3-21 20:15
Neutron Stars 1978-0-387-47301-7Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: discord 時(shí)間: 2025-3-22 01:19 作者: bleach 時(shí)間: 2025-3-22 05:53 作者: 抱怨 時(shí)間: 2025-3-22 12:27 作者: 狂怒 時(shí)間: 2025-3-22 13:22
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/n/image/664683.jpg作者: MITE 時(shí)間: 2025-3-22 19:53
https://doi.org/10.1007/978-0-387-47301-7Star; Universe; book about neutron stars; dense matter; neutron star composition; neutron star magnetic f作者: 大范圍流行 時(shí)間: 2025-3-22 23:14
Overview, ～ 1.4M⊙ and radii R ～ 10 km. Thus, their masses are close to the solar mass M⊙ = 1.989 × 10. g, but their radii are ～ 10. times smaller than the solar radius R⊙ = 6.96×10. km. Accordingly, neutron stars possess an enormous gravitational energy . and surface gravity ., . where . is the gravitational作者: 忍耐 時(shí)間: 2025-3-23 01:25
Equilibrium Plasma Properties. Outer Envelopes,oted to neutron star envelopes. These envelopes are non-uniform. The structure of an envelope for a star with the effective surface temperature ～ 10. K is schematically shown in Fig. 2.1. We indicate characteristic densities and geometrical depths of interfaces between adjoining layers. One can dist作者: arrhythmic 時(shí)間: 2025-3-23 08:50 作者: 大看臺(tái) 時(shí)間: 2025-3-23 11:38
Neutron Star Cores: Nucleons and Hyperons,of neutrons, protons, and electrons. Up to ρ ～ 2ρ. its properties can be calculated in a rather reliable way using the methods of the nuclear many-body theory, which have been applied with some success for the microscopic description of ordinary nuclear structure. At such densities the only baryons 作者: 出血 時(shí)間: 2025-3-23 17:00 作者: 熱心助人 時(shí)間: 2025-3-23 18:39 作者: 重畫(huà)只能放棄 時(shí)間: 2025-3-23 23:05 作者: 匯總 時(shí)間: 2025-3-24 05:39 作者: 巨碩 時(shí)間: 2025-3-24 10:15 作者: Corporeal 時(shí)間: 2025-3-24 14:28
en, eine zun?chst unübersehbar gro?e Zahl von Menschen get?tet und verletzt worden war, erkl?rte die spanische Regierung die baskische Terrororganisation ETA zweifelsfrei zu T?tern. Obgleich seit dem Mittag des gleichen Tages die Hinweise auf einen islamistischen Hintergrund sich verdichteten, blieb作者: 歸功于 時(shí)間: 2025-3-24 18:00 作者: 陳列 時(shí)間: 2025-3-24 21:11
en, eine zun?chst unübersehbar gro?e Zahl von Menschen get?tet und verletzt worden war, erkl?rte die spanische Regierung die baskische Terrororganisation ETA zweifelsfrei zu T?tern. Obgleich seit dem Mittag des gleichen Tages die Hinweise auf einen islamistischen Hintergrund sich verdichteten, blieb作者: 煩人 時(shí)間: 2025-3-25 01:29
nd methodology associated with the new era of photoelectric spectrometers. Over the years the aims and objectives of the Group have been broadened to include many aspects of ultraviolet and visible spectrometry. In 1973, the Group renamed itself the UV Spectrometry Group (UVSG). The techniques of fl作者: 他一致 時(shí)間: 2025-3-25 06:10 作者: 舔食 時(shí)間: 2025-3-25 11:09 作者: 憤世嫉俗者 時(shí)間: 2025-3-25 14:05 作者: Callus 時(shí)間: 2025-3-25 16:46
Equilibrium Plasma Properties. Outer Envelopes,urface temperature ～ 10. K the internal temperature of a cooling (isolated) star would be ～ 10. K; the main temperature gradient would occur in the ocean, while deeper layers would be nearly isothermal. When the star cools, the atmosphere and the ocean become thinner. In a sufficiently cold star the作者: 血統(tǒng) 時(shí)間: 2025-3-25 23:43
Textbook 2007young neutron stars, and magnetic ?elds, sometimes above 15 10 G. The present book is mainly devoted to the theory of the EOS of neutron star matter and its consequences for neutron star structure. As one moves from the neutron star surface to the center, the methods to calculate the EOS change. Ato作者: 植物群 時(shí)間: 2025-3-26 03:17 作者: Introduction 時(shí)間: 2025-3-26 07:48 作者: Factual 時(shí)間: 2025-3-26 10:07 作者: Lucubrate 時(shí)間: 2025-3-26 15:37
genen Truppen in den Irak geh?rte; was von einer gro?en Mehrheit der spanischen Bev?lkerung mit Vehemenz abgelehnt worden war. Eine islamistische T?terschaft hingegen würde den Anschlag als Folge eben dieser Beteiligung erscheinen lassen und alle Gründe und Stimmungen gegen die Beteiligung am Irak-K作者: Frequency 時(shí)間: 2025-3-26 19:53 作者: 六邊形 時(shí)間: 2025-3-26 22:25
d generates fluorescence emission spectra. In view of the increasing interest in synchronous scanning methods [1] the facility to scan both monochromators simultaneously is desirable (see also Section 7.1.3). The reflection gratings used in M1 and M2 are normally blazed to give maximum efficiencies 作者: ANT 時(shí)間: 2025-3-27 01:28
yield only indirect evidence of the pathological process. New tests are continuously being explored, implying that the ideal test for diagnosing AP and monitoring its course has not yet been established. As early as in 1952, Thistlethwaite and Hill emphasized that in order to assess the value of any作者: antidote 時(shí)間: 2025-3-27 08:25
yield only indirect evidence of the pathological process. New tests are continuously being explored, implying that the ideal test for diagnosing AP and monitoring its course has not yet been established. As early as in 1952, Thistlethwaite and Hill emphasized that in order to assess the value of any作者: conquer 時(shí)間: 2025-3-27 10:30
0067-0057 r matter and its consequences for neutron star structure. As one moves from the neutron star surface to the center, the methods to calculate the EOS change. Ato978-1-4419-2214-4978-0-387-47301-7Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: 挫敗 時(shí)間: 2025-3-27 13:51 作者: 維持 時(shí)間: 2025-3-27 20:21
Overview, constant and . is the speed of light. Clearly, neutron stars are very dense. Their mean mass density is . where ρ. = 2.8 × 10. g cm. is the so called ., the mass density of nucleon matter in heavy atomic nuclei. The central density of neutron stars is even larger, reaching (10–20) ρ.. By all means, neutron stars are . known in the Universe.作者: 偽造者 時(shí)間: 2025-3-27 22:34 作者: condescend 時(shí)間: 2025-3-28 03:09
Theory Versus Observations,s in 1967 (Chapter 1). The results obtained by the time of this writing (2006) are a tremendous challenge of observational astrophysics, but look like a failure in their essence: the EOS has been only weakly constrained by observations.作者: Firefly 時(shí)間: 2025-3-28 09:28 作者: granite 時(shí)間: 2025-3-28 13:23
0067-0057 eir theories are based on risky and far extrapolations of what we consider reliable physical theories of the structure of matter tested in laboratory. On the other hand, their observationsoffertheuniqueopportunitytotestthesetheories. Moreover, n- tronstarsareimportantdramaticpersonaeonthestageofmode作者: ostensible 時(shí)間: 2025-3-28 17:36 作者: 業(yè)余愛(ài)好者 時(shí)間: 2025-3-28 22:47
Preview of the Activities Related to , Conservation of Forest Genetic Resources in Serbiam of the . conservation of the forest genetic resources in Serbia. This form of the conservation of the forest genetic resources is the most common and the only sustainable, because the funds allocated for conservation are modest. According to the data from the current Register of Seed Facilities of作者: 不斷的變動(dòng) 時(shí)間: 2025-3-28 23:54
Christoph Strünckrtunities presented by AI and digitization in reshaping educational broadcasting. Unprecedented in its interdisciplinary approach, the book explores the intersections of communication, media, education, governm978-3-031-68532-3978-3-031-68530-9作者: peptic-ulcer 時(shí)間: 2025-3-29 05:25
Adam Graycar,Adam Jamrozikch as colchicine and the vinca alkaloids (e.g. vincristine, vinblastine). These compounds, together with podophyllotoxin and the maytansinoids (maytansine and maytanprine), possess a special affinity for tubulin, block the formation of axonal microtubules and, perhaps for these reasons, disrupt axon作者: 有害處 時(shí)間: 2025-3-29 09:55 作者: ostensible 時(shí)間: 2025-3-29 14:52
David Keavney,Charles Falcoor spaces of continuous functions and determine in particular the barrelledness character of .(.) for both, the compact-open and the pointwise topology, . being a completely regular space. Mainly for the purpose of appropriate calculation of the duals of spaces of integrable functions, we have inclu
