1993
DOI: 10.1007/bf01223802
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Zerlegung der Darboux-Drehung in Zwei Ebene Drehungen

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Cited by 6 publications
(11 citation statements)
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“…Minkowski 3-space, denoted ℝ 1 3 , is a threedimensional vector space equipped with a metric tensor <, > that provides a measure of interval or distance between events in the spacetime of special relativity. The Lorentzian metric <, > which has symmetric, bilinear and non-degenerate properties is defined as follows for vectors 𝑢 = (𝑢 1 , 𝑢 2 , 𝑢 3 ) and 𝑣 = (𝑣 1 , 𝑣 2 , 𝑣 3 ) < 𝑢, 𝑣 >= −𝑢 1 𝑣 1 + 𝑢 2 𝑣 2 + 𝑢 3 𝑣 3 .…”
Section: Preliminariesmentioning
confidence: 99%
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“…Minkowski 3-space, denoted ℝ 1 3 , is a threedimensional vector space equipped with a metric tensor <, > that provides a measure of interval or distance between events in the spacetime of special relativity. The Lorentzian metric <, > which has symmetric, bilinear and non-degenerate properties is defined as follows for vectors 𝑢 = (𝑢 1 , 𝑢 2 , 𝑢 3 ) and 𝑣 = (𝑣 1 , 𝑣 2 , 𝑣 3 ) < 𝑢, 𝑣 >= −𝑢 1 𝑣 1 + 𝑢 2 𝑣 2 + 𝑢 3 𝑣 3 .…”
Section: Preliminariesmentioning
confidence: 99%
“…A vector 𝑤 ∈ ℝ 1 3 is called spacelike vector if < 𝑤, 𝑤 >> 0 or 𝑤 = 0, timelike vector if < 𝑤, 𝑤 >< 0 or a lightlike vector if < 𝑤, 𝑤 >= 0 and 𝑤 ≠ 0. A curve 𝛾: 𝐼 ⊂ ℝ → ℝ 1 3 is called a spacelike, timelike, or lightlike curve at 𝑡 ∈ 𝐼 ⊂ ℝ if its velocity vector 𝛾′(𝑡) is a spacelike, timelike or lightlike vector, respectively (see [8,10]). Since we study the geometry of the curve, we can assign an orthonormal frame to any point on a smooth regular curve.…”
Section: Preliminariesmentioning
confidence: 99%
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