標(biāo)題: Titlebook: Nucleosynthesis and Its Implications on Nuclear and Particle Physics; Jean Audouze,Nicole Mathieu Book 1986 D. Reidel Publishing Company, [打印本頁(yè)] 作者: 重婚 時(shí)間: 2025-3-21 16:08
書(shū)目名稱(chēng)Nucleosynthesis and Its Implications on Nuclear and Particle Physics影響因子(影響力)
書(shū)目名稱(chēng)Nucleosynthesis and Its Implications on Nuclear and Particle Physics影響因子(影響力)學(xué)科排名
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書(shū)目名稱(chēng)Nucleosynthesis and Its Implications on Nuclear and Particle Physics網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱(chēng)Nucleosynthesis and Its Implications on Nuclear and Particle Physics被引頻次
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書(shū)目名稱(chēng)Nucleosynthesis and Its Implications on Nuclear and Particle Physics讀者反饋
書(shū)目名稱(chēng)Nucleosynthesis and Its Implications on Nuclear and Particle Physics讀者反饋學(xué)科排名
作者: catagen 時(shí)間: 2025-3-21 21:28
High Energy Particles in Dark Molecular Cloudsed some years ago (Meneguzzi, Audouze and Reeves (MAR) 1971) (Reeves, 1974), (Reeves and Meyer 1978). It appears that this mechanism is responsible for the production of the isotopes .Li, .Be, .B and .B for a small part of the .Li. The remaining part of this isotope has been generated in the Big Ban作者: 陶瓷 時(shí)間: 2025-3-22 00:24
Standard Big Bang Nucleosynthesis and Chemical Evolution of D and 3Hents with their primordi al abundances. It is shown that in order to reconcile the baryonic densities deduced respectively from .He and D in the frame of Standard Big Bang nucleosynthesis models, the ratio between the primordial and the present abundance of D should be as large as 7–10. This can be a作者: ligature 時(shí)間: 2025-3-22 08:33
The Survival Of Helium-3 in Starssity of nucleons, the survival of .He in the material processed through stars must be estimated. The results of detailed stellar evolution calculations which follow the destruction of .He are outlined. The survival of .He as a function of stellar mass, composition and mass loss is presented as are e作者: 微塵 時(shí)間: 2025-3-22 09:58 作者: 出血 時(shí)間: 2025-3-22 14:08
Early-Photoproduction of D And 3He and Pregalactic Nucleosynthesis of The Light Elementsedictions of the Standard Big Bang nucleosynthesis are briefly reviewed here. The first one consists in a “Big Bang photosynthesis” of D and .He induced on .He and .Li by energetic photons coming from the decay of hypothetical massive neutrinos and gravitinos: in this case the present observed D abu作者: Terminal 時(shí)間: 2025-3-22 19:32 作者: 保守 時(shí)間: 2025-3-23 00:29 作者: 繁忙 時(shí)間: 2025-3-23 05:03
Dark Matter and Cosmological Nucleosynthesis least two ad hoc assumptions. Of these more complex but complete solutions, the ability to produce large scale free structures where these dark baryons lie may be the best way to resolve the different proposed solutions to the several different dark matter problems.作者: FUME 時(shí)間: 2025-3-23 07:34 作者: 權(quán)宜之計(jì) 時(shí)間: 2025-3-23 10:13
Nucleosynthesis Accompanying Classical Nova Outburstsharacterized by substantial overabundances of the elements carbon, nitrogen, and oxygen as well as of other interesting nuclear species. Observational determinations of abundances in nova ejecta have now confirmed both that anomalous CNO enrichments do indeed occur and that the elements neon, sodium作者: 諂媚于人 時(shí)間: 2025-3-23 15:01 作者: 莊嚴(yán) 時(shí)間: 2025-3-23 19:53
Type I Supernovaeat epochs near maximum light. 2) Dynamical calculations have been done exploring the range of possible outcomes of the evolution of binary white dwarfs. 3) Consideration is given to the need to eject iron from the Galaxy to avoid overproduction by Type I events. 4) The nature of the class of peculia作者: 良心 時(shí)間: 2025-3-24 02:16
Nucleosynthesis and Type I Supernovaeignition and burning propagation. Preliminary hydrodynamic results are presented for different assumptions concerning the outcome of phase transition in cooling white dwarfs. Light curves associated with those models are shown to reproduce the “Pskovskii-Branch effect”. The possible relevance of thi作者: 云狀 時(shí)間: 2025-3-24 03:46
Explosive Nucleosynthesis in Carbon Deflagration Models of Type I SupernovaeI also indicate the existence of appreciable amounts of intermediate elements like O, Mg, Si, S, and Ca in the outer layers of the exploding star. Such an abundance pattern can be produced by carbon deflagration models of accreting carbon-oxygen white dwarfs in binary systems or stars on the asympto作者: Amendment 時(shí)間: 2025-3-24 08:44 作者: Instinctive 時(shí)間: 2025-3-24 11:16
Jean Audouze,David Lindley,Joseph Silkundierung der Thermodynamik, Grundlagen der statistischen Mechanik und Quantenmechanik, die thermodynamischen Haupts?tze und statistische Ensembles. Ein zentrales Anliegen des vorliegenden Buches ist die Diskussion der Entropie: Eine Festlegung als ein exaktes Differential in der Form von spezifisch作者: 亞麻制品 時(shí)間: 2025-3-24 15:08
R. Schaeffer,P. Delbourgo-Salvador,J. Audouzerealer Systeme.Setzt die Physik in den Vordergrund.Enge VerkDer vierte Band dieser Einführung in die theoretische Physik behandelt die statistische Physik und Thermodynamik. Themen sind dabei die statistische Fundierung der Thermodynamik, Grundlagen der statistischen Mechanik und Quantenmechanik, di作者: Carbon-Monoxide 時(shí)間: 2025-3-24 20:04
T. P. Walker,E. W. Kolb,M. S. Turnerrealer Systeme.Setzt die Physik in den Vordergrund.Enge VerkDer vierte Band dieser Einführung in die theoretische Physik behandelt die statistische Physik und Thermodynamik. Themen sind dabei die statistische Fundierung der Thermodynamik, Grundlagen der statistischen Mechanik und Quantenmechanik, di作者: 不愿 時(shí)間: 2025-3-24 23:59
David N. Schrammupplementary material: .Dieser Band beginnt mit einer vertieften Analyse von Symmetrien in der Quantenphysik. Er behandelt Quantenfeldtheorie von skalaren Feldern, Eichbosonen und Fermionen - überwiegend in kanonischer Quantisierung - und ihre Anwendungen auf wichtige elektromagnetische und schwache作者: 粗俗人 時(shí)間: 2025-3-25 03:24 作者: Deduct 時(shí)間: 2025-3-25 11:18
upplementary material: .Dieser Band beginnt mit einer vertieften Analyse von Symmetrien in der Quantenphysik. Er behandelt Quantenfeldtheorie von skalaren Feldern, Eichbosonen und Fermionen - überwiegend in kanonischer Quantisierung - und ihre Anwendungen auf wichtige elektromagnetische und schwache作者: 演講 時(shí)間: 2025-3-25 15:41
James W. Truranupplementary material: .Dieser Band beginnt mit einer vertieften Analyse von Symmetrien in der Quantenphysik. Er behandelt Quantenfeldtheorie von skalaren Feldern, Eichbosonen und Fermionen - überwiegend in kanonischer Quantisierung - und ihre Anwendungen auf wichtige elektromagnetische und schwache作者: 先行 時(shí)間: 2025-3-25 19:43
M. Wiescher,J. G?rres,F.-K. Thielemann,H. Ritterupplementary material: .Dieser Band beginnt mit einer vertieften Analyse von Symmetrien in der Quantenphysik. Er behandelt Quantenfeldtheorie von skalaren Feldern, Eichbosonen und Fermionen - überwiegend in kanonischer Quantisierung - und ihre Anwendungen auf wichtige elektromagnetische und schwache作者: 生銹 時(shí)間: 2025-3-25 23:02
R. Schaeffer,P. Delbourgo-Salvador,J. Audouzeestk?rpermodellen und die Hohlraumstrahlung besprochen. Das Buch schlie?t mit einer Diskussion realer Systeme (klassische und quantenmechanische??Vielteilchensysteme).978-3-642-12745-8978-3-642-12746-5作者: HEED 時(shí)間: 2025-3-26 03:31
T. P. Walker,E. W. Kolb,M. S. Turnerestk?rpermodellen und die Hohlraumstrahlung besprochen. Das Buch schlie?t mit einer Diskussion realer Systeme (klassische und quantenmechanische??Vielteilchensysteme).978-3-642-12745-8978-3-642-12746-5作者: acetylcholine 時(shí)間: 2025-3-26 07:25 作者: FIS 時(shí)間: 2025-3-26 10:18 作者: 敲詐 時(shí)間: 2025-3-26 13:18
Jean Audouze,David Lindley,Joseph Silkder Bose-Einstein-Kondensate) werden die Formulierung von einfachen, quantenmechanischen Festk?rpermodellen und die Hohlraumstrahlung besprochen. Das Buch schlie?t mit einer Diskussion realer Systeme (klassische und quantenmechanische??Vielteilchensysteme).作者: Overthrow 時(shí)間: 2025-3-26 19:44 作者: 移動(dòng) 時(shí)間: 2025-3-26 22:02 作者: botany 時(shí)間: 2025-3-27 03:20
B. J. Carr,W. Glatzelchanik und der -feldtheorie. Das Buch schlie?t mit Lebensdaten und historischen Anmerkungen zu einigen der Begründer der Quantenmechanik und der Quantenfeldtheorie..978-3-540-71340-1978-3-540-71341-8Series ISSN 0937-7433 Series E-ISSN 2512-5214 作者: 刪減 時(shí)間: 2025-3-27 05:44 作者: Overdose 時(shí)間: 2025-3-27 13:10
James W. Truranchanik und der -feldtheorie. Das Buch schlie?t mit Lebensdaten und historischen Anmerkungen zu einigen der Begründer der Quantenmechanik und der Quantenfeldtheorie..978-3-540-71340-1978-3-540-71341-8Series ISSN 0937-7433 Series E-ISSN 2512-5214 作者: Counteract 時(shí)間: 2025-3-27 14:47
M. Wiescher,J. G?rres,F.-K. Thielemann,H. Ritterchanik und der -feldtheorie. Das Buch schlie?t mit Lebensdaten und historischen Anmerkungen zu einigen der Begründer der Quantenmechanik und der Quantenfeldtheorie..978-3-540-71340-1978-3-540-71341-8Series ISSN 0937-7433 Series E-ISSN 2512-5214 作者: 不要嚴(yán)酷 時(shí)間: 2025-3-27 20:16 作者: alcohol-abuse 時(shí)間: 2025-3-28 01:12 作者: CRATE 時(shí)間: 2025-3-28 03:51 作者: 良心 時(shí)間: 2025-3-28 07:28 作者: browbeat 時(shí)間: 2025-3-28 10:56 作者: FILTH 時(shí)間: 2025-3-28 15:54
High Energy Particles in Dark Molecular Cloudsr the production of the isotopes .Li, .Be, .B and .B for a small part of the .Li. The remaining part of this isotope has been generated in the Big Bang and perhaps also in stellar processes. I have reviewed the situation in my paper “Primordial Nucleosynthesis in 1985” in this Moriond 1985 volume (paper I).作者: Cervical-Spine 時(shí)間: 2025-3-28 22:05 作者: 衰弱的心 時(shí)間: 2025-3-29 01:15
The Survival Of Helium-3 in Starss which follow the destruction of .He are outlined. The survival of .He as a function of stellar mass, composition and mass loss is presented as are estimates of the primordial abundances of D and .He; the cosmological consequences are summarized.作者: Ischemic-Stroke 時(shí)間: 2025-3-29 07:06
Nucleosynthesis and Type I Supernovaein cooling white dwarfs. Light curves associated with those models are shown to reproduce the “Pskovskii-Branch effect”. The possible relevance of this to the determination of Hubble’s constant and ways to avoid overproduction of .Fe are finally discussed.作者: mucous-membrane 時(shí)間: 2025-3-29 08:47 作者: 來(lái)自于 時(shí)間: 2025-3-29 12:01 作者: Eructation 時(shí)間: 2025-3-29 19:14
1389-2185 Overview: 978-94-010-8534-2978-94-009-4578-4Series ISSN 1389-2185 作者: 星球的光亮度 時(shí)間: 2025-3-29 21:45 作者: 調(diào)整校對(duì) 時(shí)間: 2025-3-30 02:24
Differentially Rotating Equilibrium Models and the Collapse of Rotating Degenerate ConfigurationsUsing a recently developed method (Erlguchl and Müller, 1985a) two kind of problems involving axisymmetric, differentially rotating degenerate configurations are investigated:作者: organism 時(shí)間: 2025-3-30 08:05
Nato Science Series C:http://image.papertrans.cn/n/image/668807.jpg作者: bourgeois 時(shí)間: 2025-3-30 09:32 作者: Annotate 時(shí)間: 2025-3-30 12:38 作者: Overstate 時(shí)間: 2025-3-30 18:19
Primordial Nucleosynthesis with Generic Particlesduction of .He and D + .He is calculated as a function of the mass, spin degrees of freedom, and spin statistics of the generic particle for masses in the range 10. ? m/m. ? 10.. The particular case of the Gelmini and Roncadelli majoron model for massive neutrinos is discussed.作者: 暴發(fā)戶 時(shí)間: 2025-3-30 21:58
Dark Matter and Cosmological Nucleosynthesis least two ad hoc assumptions. Of these more complex but complete solutions, the ability to produce large scale free structures where these dark baryons lie may be the best way to resolve the different proposed solutions to the several different dark matter problems.作者: Amenable 時(shí)間: 2025-3-31 01:30 作者: coalition 時(shí)間: 2025-3-31 05:13
Reaction Rates in the RP-Process and Nucleosynthesis in Novaeve hydrogen burning. These rates were applied in a systematic analysis for a variety of temperature conditions, appropriate to nova explosions, to study nucleosynthesis for isotopes of Ne Na Mg Al Si. The results are discussed in comparison with recent observations of elemental abundances in nova ejecta.作者: IRK 時(shí)間: 2025-3-31 11:32
Type I Supernovaeat epochs near maximum light. 2) Dynamical calculations have been done exploring the range of possible outcomes of the evolution of binary white dwarfs. 3) Consideration is given to the need to eject iron from the Galaxy to avoid overproduction by Type I events. 4) The nature of the class of peculiar Type I supernovae is explored.作者: esthetician 時(shí)間: 2025-3-31 15:45
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