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A Remark About the “Geodesic Principle” in General Relativity

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Book cover Analysis and Interpretation in the Exact Sciences

Part of the book series: The Western Ontario Series in Philosophy of Science ((WONS,volume 78))

Abstract

It is often claimed that the geodesic principle can be recovered as a theorem in general relativity. Indeed, it is claimed that it is a consequence of Einstein’s equation (via the conservation principle that is, itself, a consequence of that equation). These claims are certainly correct, but it may be worth drawing attention to one small qualification. Though the geodesic principle can be recovered as theorem in general relativity, it is not a consequence of Einstein’s equation (or the conservation principle) alone. Other assumptions are needed to drive the theorems in question. My goal in this short note is to make this claim precise.

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Notes

  1. 1.

    We will assume familiarity with the basic mathematical formalism of general relativity in what follows. For background material, see, e.g., Hawking and Ellis (1972), Wald (1984), or Malament (2012).

  2. 2.

    All the material in the section is perfectly standard except for one small bit of ad hoc terminology. In addition to the weak and dominant energy conditions, we will consider something that we call the “strengthened dominant energy condition.”

  3. 3.

    This is not a standard name.

  4. 4.

    If λ a is a smooth spacelike field, then \(T_{ab} = \lambda _a \lambda _b\) satisfies the weak, but not the dominant, energy condition. Similarly, if λ a is a smooth, non-vanishing null field, then \(T_{ab} = \lambda _a \lambda_b\) satisfies the dominant, but not the strengthened dominant, energy condition.

  5. 5.

    Let \(\gamma :\;I \to M\) be a smooth curve. We say that a point p in M is a future-endpoint of γ if, for all open sets O containing p, there exists an s 0 in I such that for all \(s \in I\), if \(s \ge s_0\), then \({{\upgamma} \left(\textrm{s}\right)} \in O\), i.e. the image of γ eventually enters and remains in O. (Past-endpoints are defined similarly.)

  6. 6.

    For a proof, see Hawking and Ellis (1972, p. 94).

  7. 7.

    See, for example, proposition 1.7.11 in Malament (2012).

References

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Acknowledgements

I am grateful to Robert Geroch for giving me the basic idea for the counterexample (Proposition 3) that is the principal point of interest in this note. Thanks also to Harvey Brown, Erik Curiel, John Earman, David Garfinkle, John Manchak, Wayne Myrvold, John Norton, and Jim Weatherall for comments on an earlier draft.

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Correspondence to David B. Malament .

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Malament, D.B. (2012). A Remark About the “Geodesic Principle” in General Relativity. In: Frappier, M., Brown, D., DiSalle, R. (eds) Analysis and Interpretation in the Exact Sciences. The Western Ontario Series in Philosophy of Science, vol 78. Springer, Dordrecht. https://doi.org/10.1007/978-94-007-2582-9_14

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