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宇宙“常数”变化的Bianchi-Ⅰ型宇宙模型的解 被引量:2
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作者 王行翔 《安徽师范大学学报(自然科学版)》 CAS 2004年第3期280-282,共3页
在定域旋转对称的Bianchi-Ⅰ型时空中讨论了宇宙"常数"为变量的Einstein引力场方程的解.从能量动量守恒定律中包括真空的能量-动量T(vac)μν=-Λ(t)gμν的观点出发,得到了场方程的一个精确解,并对其相关的物理性质作了简要... 在定域旋转对称的Bianchi-Ⅰ型时空中讨论了宇宙"常数"为变量的Einstein引力场方程的解.从能量动量守恒定律中包括真空的能量-动量T(vac)μν=-Λ(t)gμν的观点出发,得到了场方程的一个精确解,并对其相关的物理性质作了简要的讨论.这是一个较为普遍的解,它把文献中的结果作为特例包括在内. 展开更多
关键词 常数 场方程 定域 精确解 引力场 宇宙模型 旋转对称 特例 动量守恒定律 观点
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Lepton-number-violating decays of singly-charged Higgs bosons in the type-(Ⅰ+Ⅱ) seesaw model
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作者 任凭 邢志忠 《Chinese Physics C》 SCIE CAS CSCD 2010年第4期433-443,共11页
The lepton-number-violating decays of singly-charged Higgs bosons H^± are investigated in the minimal type-( Ⅰ+Ⅱ ) seesaw model with one SU(2)L Higgs triplet △ and one heavy Majorana neutrino N1 at the Te... The lepton-number-violating decays of singly-charged Higgs bosons H^± are investigated in the minimal type-( Ⅰ+Ⅱ ) seesaw model with one SU(2)L Higgs triplet △ and one heavy Majorana neutrino N1 at the TeV scale. We find that the branching ratios B(H^+ → 1α^+υ^-) (for α = e,μ,τ) depend not only on the mass and mixing parameters of three light neutrinos υi (for i = 1, 2, 3) but also on those of N1. Assuming that the mass of N1 lies in the range of 200 GeV to 1 TeV, we figure out the generous interference bands for the contributions of υi and N1 to B(H^+→ 1α^+υ^-). We illustrate some salient features of such interference effects by considering three typical mass patterns of υi, and show that the relevant Majorana CP-violating phases can affect the magnitudes of B(H^+→ 1α^+υ^-)) in this parameter region. 展开更多
关键词 type-+Ⅱ seesaw model Higgs triplet lepton number violation
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Energy Conditions and Conservation Laws in LRS Bianchi Type Ⅰ Spacetimes via Noether Symmetries
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作者 Sumaira Saleem Akhtar Tahir Hussain 《Communications in Theoretical Physics》 SCIE CAS CSCD 2019年第3期298-306,共9页
In this paper, we have completely classified the locally rotationally symmetric(LRS) Bianchi Type Ⅰ spacetimes via Noether symmetries(NS). The usual Lagrangian corresponding to LRS Bianchi Type Ⅰ metric is used to f... In this paper, we have completely classified the locally rotationally symmetric(LRS) Bianchi Type Ⅰ spacetimes via Noether symmetries(NS). The usual Lagrangian corresponding to LRS Bianchi Type Ⅰ metric is used to find the set of determining equations. To achieve a complete classification, these determining equations are generally integrated to find the components of NS vector field and the metric coefficients. During this procedure, several cases arise which give different Noether algebras of dimension 5,..., 9, 11, and 17. A comparison is established between the obtained NS and the Killing and homothetic vectors. Corresponding to all NS generators, the conservation laws are stated by using Noether's theorem. The metrics which we have obtained as a result of our classification are shown to be anisotropic or perfect fluids which satisfy certain energy conditions. 展开更多
关键词 bianchi type model Noether symmetry conservation Laws energy conditions
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