標(biāo)題: Titlebook: Gauge Theory and the Early Universe; P. Galeotti,David N. Schramm Book 1988 Kluwer Academic Publishers 1988 Cosmology.Dark matter.Gravity. [打印本頁(yè)] 作者: 預(yù)兆前 時(shí)間: 2025-3-21 18:32
書(shū)目名稱Gauge Theory and the Early Universe影響因子(影響力)
書(shū)目名稱Gauge Theory and the Early Universe影響因子(影響力)學(xué)科排名
書(shū)目名稱Gauge Theory and the Early Universe網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱Gauge Theory and the Early Universe網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱Gauge Theory and the Early Universe被引頻次
書(shū)目名稱Gauge Theory and the Early Universe被引頻次學(xué)科排名
書(shū)目名稱Gauge Theory and the Early Universe年度引用
書(shū)目名稱Gauge Theory and the Early Universe年度引用學(xué)科排名
書(shū)目名稱Gauge Theory and the Early Universe讀者反饋
書(shū)目名稱Gauge Theory and the Early Universe讀者反饋學(xué)科排名
作者: 圣歌 時(shí)間: 2025-3-22 00:13 作者: CYT 時(shí)間: 2025-3-22 00:33
Galaxy Formation in Cold Dark Matter Dominated Universes: Observational Tests,critical density: .. ≡ 3../[8.] = 2 · 10. h. g cm.; .. is the Hubble constant and h = H. /[100 km s. Mpc.]. If Ω. is less than or equal to unity (open or flat model respectively), the universe will expand forever; if Ω. is greater than unity, the universe will recollapse eventually.作者: arsenal 時(shí)間: 2025-3-22 07:31
Phenomenology And Cosmology With Superstring Motivated Models,xion. The existence of topologically stable superconducting vortices (strings), surviving until today, is predicted. Other topics that are discussed include proton decay, the baryon asymmetry in the Universe and n - n oscillations.作者: 樹(shù)木心 時(shí)間: 2025-3-22 09:48
: Australianising HBO-Style Television?ology, the study of the early evolution of the universe. The range of parameters (dimensions, temperatures, densities, etc..) to be taken into account in cosmology is so vast that one is forced to use theories or experimental data of wide ranging origin. This is demonstrated in the following few examples.作者: 惡臭 時(shí)間: 2025-3-22 15:53
,Elma Kelly’s Empire: An Australian in Asia,n S0(10) model, for example, magnetic monopoles with mass ~ 10. – 10. GeV can occur at a level which is experimentally detectable. The topologically unstable string - wall system of axion models provides an important source of density fluctuations as a consequence of inflation.作者: 惡臭 時(shí)間: 2025-3-22 19:17
Austrian Economics in Transition We show that for an adiabatic evolving meanfield ? (t) there arises the derivative of the effective potential as well as a local damping term proportional to ? , which has its origin in the fact that particles which will be created by the time dependence of the meanfield will decay subsequently into lighter particles.作者: 極深 時(shí)間: 2025-3-22 23:57
Austrian National Socialism before 1918 the t,? submanifold as a consequence of the field equations. This justifies the usual assumption that the geometry of the 5th coordinate is a circle. It is shown they are equivalent to the Lorenz - Petzold type (ix) solutions.作者: 浮夸 時(shí)間: 2025-3-23 02:35 作者: Processes 時(shí)間: 2025-3-23 07:00 作者: 大門(mén)在匯總 時(shí)間: 2025-3-23 10:23
Monopoles and Axions in an Inflationary Universe,n S0(10) model, for example, magnetic monopoles with mass ~ 10. – 10. GeV can occur at a level which is experimentally detectable. The topologically unstable string - wall system of axion models provides an important source of density fluctuations as a consequence of inflation.作者: CRUE 時(shí)間: 2025-3-23 16:01 作者: 愛(ài)社交 時(shí)間: 2025-3-23 20:21
Constraints on the Geometry of the 5th dimension in cosmological solutions of Five dimensional Rela the t,? submanifold as a consequence of the field equations. This justifies the usual assumption that the geometry of the 5th coordinate is a circle. It is shown they are equivalent to the Lorenz - Petzold type (ix) solutions.作者: 紀(jì)念 時(shí)間: 2025-3-24 01:36 作者: 惰性氣體 時(shí)間: 2025-3-24 02:44 作者: antidepressant 時(shí)間: 2025-3-24 08:32
https://doi.org/10.1007/978-1-349-11801-4itational field,I calculate the time-evolution of the cosmic scale factor and of the scalar field in the case of a λ?. theory,in order to understand when a λ?. theory is able to drive inflation.Some new topics are mentioned,too.作者: 男學(xué)院 時(shí)間: 2025-3-24 11:26
Cosmology and Extra Dimensions,However, if the big bang is extrapolated back to the Planck time, then the characteristic size of . internal and external dimensions were the same, and the internal dimensions may have had a more direct role in the dynamics of the evolution of the Universe. This chapter presents some speculations about the role of extra dimensions in cosmology.作者: Prosaic 時(shí)間: 2025-3-24 14:54 作者: Constant 時(shí)間: 2025-3-24 20:59 作者: Palpitation 時(shí)間: 2025-3-25 02:31
: Australianising HBO-Style Television? connected with the new ideas and developments in the other field. Roughly speaking, many different subdisciplines of physics seem to converge in cosmology, the study of the early evolution of the universe. The range of parameters (dimensions, temperatures, densities, etc..) to be taken into account作者: HAVOC 時(shí)間: 2025-3-25 03:22 作者: candle 時(shí)間: 2025-3-25 09:55
Fred Cahir,Sara Weuffen,Jo Caminitial cosmological perturbations due to the parametric effect is considered. The related fluctuations of the relic background radiation are analysed. The spottiness structure of the large-scale background anisotropy is discussed.作者: 雄偉 時(shí)間: 2025-3-25 13:55
Rosemary Berreen,Michael Wearingcrowave background (CMB), and the agreement between the predictions of the primordial nucleosynthesis theories and the observed abundance of light elements. The cosmological Friedmann models are parametrized by the density parameter Ω.. This measures the present cosmological density in units of the 作者: Transfusion 時(shí)間: 2025-3-25 18:58 作者: 向宇宙 時(shí)間: 2025-3-25 22:54 作者: 侵害 時(shí)間: 2025-3-26 00:08
https://doi.org/10.1007/978-981-15-6145-0the universe seem to be placing severe constraints on cosmological models. In addition, it is shown that the bulk of the baryonic matter is also dark and must be accounted for as well. The nucleosynthesis arguments are now strongly supported by high energy collider experiments as well as astronomica作者: 聲音刺耳 時(shí)間: 2025-3-26 07:38 作者: Comedienne 時(shí)間: 2025-3-26 08:34
https://doi.org/10.1007/978-1-349-21163-0may have condensed into the galactic halo. These detectors are based on the principle, due to Sikivie [1], of conversion of axions to microwave photons in a magnetic field. We describe the device built by a Rochester-Brookhaven-Fermilab collaboration*, its sensitivity, and the motivation from astrop作者: 鬧劇 時(shí)間: 2025-3-26 13:56 作者: oncologist 時(shí)間: 2025-3-26 20:23 作者: boisterous 時(shí)間: 2025-3-26 22:04
https://doi.org/10.1007/978-1-349-11801-4pacelike three-surface S obeys a zero energy Schr?dinger equation,the Wheeler-De Witt equation for closed universes. . may be given by a functional integral taken over all compact euclidean fourmetrics which have a boundary at S, and over all field configurations which match the given value on S.Aft作者: 打谷工具 時(shí)間: 2025-3-27 02:29
https://doi.org/10.1057/9781137368805hronous reference system will tend asymptotically in time towards the de Sitter solution, so making the problem of initial conditions less severe. The implications for inflationary scenarios are examined and it is found that after inflation the universe stays isotropic and homogeneous for a very lon作者: 試驗(yàn) 時(shí)間: 2025-3-27 06:44 作者: Breach 時(shí)間: 2025-3-27 11:41 作者: 精密 時(shí)間: 2025-3-27 15:58
https://doi.org/10.1007/978-1-349-21163-0may have condensed into the galactic halo. These detectors are based on the principle, due to Sikivie [1], of conversion of axions to microwave photons in a magnetic field. We describe the device built by a Rochester-Brookhaven-Fermilab collaboration*, its sensitivity, and the motivation from astrophysics for attempting to observe axions.作者: ANIM 時(shí)間: 2025-3-27 17:57
https://doi.org/10.1057/9781137368805hronous reference system will tend asymptotically in time towards the de Sitter solution, so making the problem of initial conditions less severe. The implications for inflationary scenarios are examined and it is found that after inflation the universe stays isotropic and homogeneous for a very long time.作者: 斜坡 時(shí)間: 2025-3-28 00:29
The Problem of Origin of the Primordial Cosmological Perturbations,al cosmological perturbations due to the parametric effect is considered. The related fluctuations of the relic background radiation are analysed. The spottiness structure of the large-scale background anisotropy is discussed.作者: 向前變橢圓 時(shí)間: 2025-3-28 04:11
An Experimental Search for Galactic Axions,may have condensed into the galactic halo. These detectors are based on the principle, due to Sikivie [1], of conversion of axions to microwave photons in a magnetic field. We describe the device built by a Rochester-Brookhaven-Fermilab collaboration*, its sensitivity, and the motivation from astrophysics for attempting to observe axions.作者: aggressor 時(shí)間: 2025-3-28 08:09 作者: BLA 時(shí)間: 2025-3-28 13:35 作者: 支柱 時(shí)間: 2025-3-28 15:40 作者: cacophony 時(shí)間: 2025-3-28 19:57 作者: Mundane 時(shí)間: 2025-3-29 00:32
Australia and Latin America in a Global Era,The emergence of structures and complexity in the expanding universe is related to the existence of sources of entropy and information (stocked entropy). The physical processes responsible for these phenomena are reviewed and situated in their chronological order.作者: 不透明 時(shí)間: 2025-3-29 04:42 作者: Embolic-Stroke 時(shí)間: 2025-3-29 09:16
Australia’s Toxic Medical CultureAnisotropy measurement techniques and results are reviewed, with special attention given to experimental problems..The cosmological relevance of the dipole anisotropy, the only anisotropy truly detected in the Cosmic Background Radiation, is discussed.作者: Promotion 時(shí)間: 2025-3-29 12:09 作者: 傻 時(shí)間: 2025-3-29 17:31
https://doi.org/10.1057/9781137368843I review the model of Chaotic Inflation driven by the corrections to Einstein’s gravity quadratic in curvature. Initial fluctuations are discussed using particular solution of the Wheeler-De Witt equation. The coefficient of the quadratic term is restricted to be between 10. and 10. G.作者: 不易燃 時(shí)間: 2025-3-29 21:12
,Cosmic Information and the “Anthropic” Principle,The emergence of structures and complexity in the expanding universe is related to the existence of sources of entropy and information (stocked entropy). The physical processes responsible for these phenomena are reviewed and situated in their chronological order.作者: paleolithic 時(shí)間: 2025-3-30 02:20
Trends in the Astrophysics of Light Elements: Cosmology and Stellar Physics,The properties ( nuclear, atomic, molecular ) of the light elements H, He, and Li are known well enough to warrant the study of many astrophysical processes through their abundance determinations. In this paper I plan to review three domains in which this situation applies:作者: 邊緣 時(shí)間: 2025-3-30 07:30 作者: 結(jié)合 時(shí)間: 2025-3-30 08:27 作者: 閃光你我 時(shí)間: 2025-3-30 13:22
,, Inflation,I review the model of Chaotic Inflation driven by the corrections to Einstein’s gravity quadratic in curvature. Initial fluctuations are discussed using particular solution of the Wheeler-De Witt equation. The coefficient of the quadratic term is restricted to be between 10. and 10. G.作者: 客觀 時(shí)間: 2025-3-30 19:22
Gauge Theory and the Early Universe, connected with the new ideas and developments in the other field. Roughly speaking, many different subdisciplines of physics seem to converge in cosmology, the study of the early evolution of the universe. The range of parameters (dimensions, temperatures, densities, etc..) to be taken into account作者: preservative 時(shí)間: 2025-3-30 21:58 作者: 決定性 時(shí)間: 2025-3-31 00:56
The Problem of Origin of the Primordial Cosmological Perturbations,al cosmological perturbations due to the parametric effect is considered. The related fluctuations of the relic background radiation are analysed. The spottiness structure of the large-scale background anisotropy is discussed.作者: Mitigate 時(shí)間: 2025-3-31 05:25 作者: Injunction 時(shí)間: 2025-3-31 11:32 作者: Mast-Cell 時(shí)間: 2025-3-31 14:47 作者: PLUMP 時(shí)間: 2025-3-31 20:22
The Consistency Problems of Large Scale Structure, Dark Matter, and Galaxy Formation,the universe seem to be placing severe constraints on cosmological models. In addition, it is shown that the bulk of the baryonic matter is also dark and must be accounted for as well. The nucleosynthesis arguments are now strongly supported by high energy collider experiments as well as astronomica作者: 輕浮思想 時(shí)間: 2025-3-31 21:45 作者: CHARM 時(shí)間: 2025-4-1 05:10 作者: Vital-Signs 時(shí)間: 2025-4-1 08:44
On the Effective Evolution Equation of the Scalar Field in the New Inflationary Universe,ive calculation scheme proposed recently by M. Morikawa and M. Sasaki. The expectation value ? of the scalar field is allowed to be dependent on time. We show that for an adiabatic evolving meanfield ? (t) there arises the derivative of the effective potential as well as a local damping term proport作者: cutlery 時(shí)間: 2025-4-1 13:44
Constraints on the Geometry of the 5th dimension in cosmological solutions of Five dimensional Relaand general dependence of the metric on time t, as well as on the 5. coordinate ?..Such solutions are shown to exibit always a killing vector field in the t,? submanifold as a consequence of the field equations. This justifies the usual assumption that the geometry of the 5th coordinate is a circle.
