<p>We establish the nonlinear stability to the future of tilted two-fluid Bianchi I solutions to the Einstein–Euler equations with positive cosmological constant and linear equations of state <InlineEquation ID="IEq1"> <EquationSource Format="TEX">\(p_{(\mathfrak {a})}=K_{(\mathfrak {a})}\rho _{(\mathfrak {a})}\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msub> <mi>p</mi> <mrow> <mo stretchy="false">(</mo> <mi mathvariant="fraktur">a</mi> <mo stretchy="false">)</mo> </mrow> </msub> <mo>=</mo> <msub> <mi>K</mi> <mrow> <mo stretchy="false">(</mo> <mi mathvariant="fraktur">a</mi> <mo stretchy="false">)</mo> </mrow> </msub> <msub> <mi>ρ</mi> <mrow> <mo stretchy="false">(</mo> <mi mathvariant="fraktur">a</mi> <mo stretchy="false">)</mo> </mrow> </msub> </mrow> </math></EquationSource> </InlineEquation>, <InlineEquation ID="IEq2"> <EquationSource Format="TEX">\(\mathfrak {a}\in \{1,2\}\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi mathvariant="fraktur">a</mi> <mo>∈</mo> <mo stretchy="false">{</mo> <mn>1</mn> <mo>,</mo> <mn>2</mn> <mo stretchy="false">}</mo> </mrow> </math></EquationSource> </InlineEquation>, where <InlineEquation ID="IEq3"> <EquationSource Format="TEX">\(\frac{1}{3}&lt;K_{(\mathfrak {a})}&lt;\frac{5}{7}\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mfrac> <mn>1</mn> <mn>3</mn> </mfrac> <mo>&lt;</mo> <msub> <mi>K</mi> <mrow> <mo stretchy="false">(</mo> <mi mathvariant="fraktur">a</mi> <mo stretchy="false">)</mo> </mrow> </msub> <mo>&lt;</mo> <mfrac> <mn>5</mn> <mn>7</mn> </mfrac> </mrow> </math></EquationSource> </InlineEquation>.</p>

错误:搜索内容不能为空,请输入英文关键词
错误:关键词超出字数限制,请精简
高级检索

Future Stability of Tilted Two-Fluid Bianchi I Spacetimes

  • Grigorios Fournodavlos,
  • Elliot Marshall,
  • Todd A. Oliynyk

摘要

We establish the nonlinear stability to the future of tilted two-fluid Bianchi I solutions to the Einstein–Euler equations with positive cosmological constant and linear equations of state \(p_{(\mathfrak {a})}=K_{(\mathfrak {a})}\rho _{(\mathfrak {a})}\) p ( a ) = K ( a ) ρ ( a ) , \(\mathfrak {a}\in \{1,2\}\) a { 1 , 2 } , where \(\frac{1}{3}<K_{(\mathfrak {a})}<\frac{5}{7}\) 1 3 < K ( a ) < 5 7 .