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In terms of spin coefficients, shear is defined as σ = (m_a)( m_b)(∇_a l^b) ,

$$\sigma=(m_a)(m_b)(\nabla_al^b)$$

where m,l$m,l$ denotes null tetrad vectors. I came across the following paragraph from one of Stephen Hawking's papers - "What happens is that the perturbation produces tidal forces which distort the horizon. If the black hole is not rotating, the distortion of an element of the horizon will be constant in time and the shear will be zero. If the black hole is rotating, however, distortion will be periodic in time and so there will be shear". Soone of Stephen Hawking's papers:

What happens is that the perturbation produces tidal forces which distort the horizon. If the black hole is not rotating, the distortion of an element of the horizon will be constant in time and the shear will be zero. If the black hole is rotating, however, distortion will be periodic in time and so there will be shear.

So distortion directly does not mean shear? In a nonrotating black hole, though distortion is constant in time, still, distortion is there, then why shear is zero?

In terms of spin coefficients, shear is defined as σ = (m_a)( m_b)(∇_a l^b) , where m,l denotes null tetrad vectors. I came across the following paragraph from one of Stephen Hawking's papers - "What happens is that the perturbation produces tidal forces which distort the horizon. If the black hole is not rotating, the distortion of an element of the horizon will be constant in time and the shear will be zero. If the black hole is rotating, however, distortion will be periodic in time and so there will be shear". So distortion directly does not mean shear? In a nonrotating black hole, though distortion is constant in time, still, distortion is there, then why shear is zero?

In terms of spin coefficients, shear is defined as

$$\sigma=(m_a)(m_b)(\nabla_al^b)$$

where $m,l$ denotes null tetrad vectors. I came across the following paragraph from one of Stephen Hawking's papers:

What happens is that the perturbation produces tidal forces which distort the horizon. If the black hole is not rotating, the distortion of an element of the horizon will be constant in time and the shear will be zero. If the black hole is rotating, however, distortion will be periodic in time and so there will be shear.

So distortion directly does not mean shear? In a nonrotating black hole, though distortion is constant in time, still, distortion is there, then why shear is zero?

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Shear on the event horizon of the black hole

In terms of spin coefficients, shear is defined as σ = (m_a)( m_b)(∇_a l^b) , where m,l denotes null tetrad vectors. I came across the following paragraph from one of Stephen Hawking's papers - "What happens is that the perturbation produces tidal forces which distort the horizon. If the black hole is not rotating, the distortion of an element of the horizon will be constant in time and the shear will be zero. If the black hole is rotating, however, distortion will be periodic in time and so there will be shear". So distortion directly does not mean shear? In a nonrotating black hole, though distortion is constant in time, still, distortion is there, then why shear is zero?