<p>In this article, we study space-like and time-like surfaces in a Robertson-Walker space-time, denoted by <InlineEquation ID="IEq1"> <EquationSource Format="TEX">\(L^4_1(f,c)\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msubsup> <mi>L</mi> <mn>1</mn> <mn>4</mn> </msubsup> <mrow> <mo stretchy="false">(</mo> <mi>f</mi> <mo>,</mo> <mi>c</mi> <mo stretchy="false">)</mo> </mrow> </mrow> </math></EquationSource> </InlineEquation>, having positive relative nullity. First, we give the necessary and sufficient conditions for such space-like and time-like surfaces in <InlineEquation ID="IEq2"> <EquationSource Format="TEX">\(L^4_1(f,c)\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msubsup> <mi>L</mi> <mn>1</mn> <mn>4</mn> </msubsup> <mrow> <mo stretchy="false">(</mo> <mi>f</mi> <mo>,</mo> <mi>c</mi> <mo stretchy="false">)</mo> </mrow> </mrow> </math></EquationSource> </InlineEquation>. Then, we obtain the local classification theorems for space-like and time-like surfaces in <InlineEquation ID="IEq3"> <EquationSource Format="TEX">\(L^4_1(f,0)\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msubsup> <mi>L</mi> <mn>1</mn> <mn>4</mn> </msubsup> <mrow> <mo stretchy="false">(</mo> <mi>f</mi> <mo>,</mo> <mn>0</mn> <mo stretchy="false">)</mo> </mrow> </mrow> </math></EquationSource> </InlineEquation> with positive relative nullity, where the second factor is 3-dimensional Euclidean space. Finally, we consider the space-like and time-like surfaces in <InlineEquation ID="IEq4"> <EquationSource Format="TEX">\(\mathbb {E}^1_1\times \mathbb {S}^3\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msubsup> <mrow> <mi mathvariant="double-struck">E</mi> </mrow> <mn>1</mn> <mn>1</mn> </msubsup> <mo>×</mo> <msup> <mrow> <mi mathvariant="double-struck">S</mi> </mrow> <mn>3</mn> </msup> </mrow> </math></EquationSource> </InlineEquation> and <InlineEquation ID="IEq5"> <EquationSource Format="TEX">\(\mathbb {E}^1_1\times \mathbb {H}^3\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msubsup> <mrow> <mi mathvariant="double-struck">E</mi> </mrow> <mn>1</mn> <mn>1</mn> </msubsup> <mo>×</mo> <msup> <mrow> <mi mathvariant="double-struck">H</mi> </mrow> <mn>3</mn> </msup> </mrow> </math></EquationSource> </InlineEquation> with positive relative nullity. These are the special spaces of <InlineEquation ID="IEq6"> <EquationSource Format="TEX">\(L^4_1(f,c)\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msubsup> <mi>L</mi> <mn>1</mn> <mn>4</mn> </msubsup> <mrow> <mo stretchy="false">(</mo> <mi>f</mi> <mo>,</mo> <mi>c</mi> <mo stretchy="false">)</mo> </mrow> </mrow> </math></EquationSource> </InlineEquation> when the warping function <i>f</i> is a constant function, with <InlineEquation ID="IEq7"> <EquationSource Format="TEX">\(c=1\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>c</mi> <mo>=</mo> <mn>1</mn> </mrow> </math></EquationSource> </InlineEquation> for <InlineEquation ID="IEq8"> <EquationSource Format="TEX">\(\mathbb {E}^1_1\times \mathbb {S}^3\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msubsup> <mrow> <mi mathvariant="double-struck">E</mi> </mrow> <mn>1</mn> <mn>1</mn> </msubsup> <mo>×</mo> <msup> <mrow> <mi mathvariant="double-struck">S</mi> </mrow> <mn>3</mn> </msup> </mrow> </math></EquationSource> </InlineEquation> and <InlineEquation ID="IEq9"> <EquationSource Format="TEX">\(c=-1\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>c</mi> <mo>=</mo> <mo>-</mo> <mn>1</mn> </mrow> </math></EquationSource> </InlineEquation> for <InlineEquation ID="IEq10"> <EquationSource Format="TEX">\(\mathbb {E}^1_1\times \mathbb {H}^3\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msubsup> <mrow> <mi mathvariant="double-struck">E</mi> </mrow> <mn>1</mn> <mn>1</mn> </msubsup> <mo>×</mo> <msup> <mrow> <mi mathvariant="double-struck">H</mi> </mrow> <mn>3</mn> </msup> </mrow> </math></EquationSource> </InlineEquation>.</p>

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Surfaces in Robertson-Walker Space-Times with Positive Relative Nullity

  • Burcu Bektaş Demirci,
  • Nurettin Cenk Turgay

摘要

In this article, we study space-like and time-like surfaces in a Robertson-Walker space-time, denoted by \(L^4_1(f,c)\) L 1 4 ( f , c ) , having positive relative nullity. First, we give the necessary and sufficient conditions for such space-like and time-like surfaces in \(L^4_1(f,c)\) L 1 4 ( f , c ) . Then, we obtain the local classification theorems for space-like and time-like surfaces in \(L^4_1(f,0)\) L 1 4 ( f , 0 ) with positive relative nullity, where the second factor is 3-dimensional Euclidean space. Finally, we consider the space-like and time-like surfaces in \(\mathbb {E}^1_1\times \mathbb {S}^3\) E 1 1 × S 3 and \(\mathbb {E}^1_1\times \mathbb {H}^3\) E 1 1 × H 3 with positive relative nullity. These are the special spaces of \(L^4_1(f,c)\) L 1 4 ( f , c ) when the warping function f is a constant function, with \(c=1\) c = 1 for \(\mathbb {E}^1_1\times \mathbb {S}^3\) E 1 1 × S 3 and \(c=-1\) c = - 1 for \(\mathbb {E}^1_1\times \mathbb {H}^3\) E 1 1 × H 3 .