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| Natura: | Preprint |
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2026
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| Accesso online: | https://arxiv.org/abs/2604.06292 |
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| _version_ | 1866917389165133824 |
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| author | Lorek, Krzysztof Louko, Jorma Dragan, Andrzej |
| author_facet | Lorek, Krzysztof Louko, Jorma Dragan, Andrzej |
| contents | For a quantum scalar field that is confined in a uniformly linearly accelerated cavity in Minkowski spacetime and interacts linearly with a scalar field that is not confined in the cavity, a de-excitation probability formula was obtained in [1] [K. Lorek et al, Class. Quant. Grav. 32, 175003 (2015) [arXiv:1503.01025]] by a first-order perturbation theory calculation. A recent Comment [2] [V. Toussaint, Class. Quant. Grav. 43, 068001 (2026)] questions this formula on the grounds that the calculation in [1] invokes Rindler modes both in the Rindler wedge of the accelerated cavity and in the opposing, causally disconnected Rindler wedge. In the present Reply we rederive the de-excitation formula given in [1] by a perturbation theory calculation that is formulated entirely within the Rindler wedge of the accelerated cavity. We also take the opportunity to comment on the role of the two sets of Rindler modes in the calculation presented in [1]. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2604_06292 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Reply to 'Comment on "Ideal clocks -- a convenient fiction'' ' Lorek, Krzysztof Louko, Jorma Dragan, Andrzej General Relativity and Quantum Cosmology For a quantum scalar field that is confined in a uniformly linearly accelerated cavity in Minkowski spacetime and interacts linearly with a scalar field that is not confined in the cavity, a de-excitation probability formula was obtained in [1] [K. Lorek et al, Class. Quant. Grav. 32, 175003 (2015) [arXiv:1503.01025]] by a first-order perturbation theory calculation. A recent Comment [2] [V. Toussaint, Class. Quant. Grav. 43, 068001 (2026)] questions this formula on the grounds that the calculation in [1] invokes Rindler modes both in the Rindler wedge of the accelerated cavity and in the opposing, causally disconnected Rindler wedge. In the present Reply we rederive the de-excitation formula given in [1] by a perturbation theory calculation that is formulated entirely within the Rindler wedge of the accelerated cavity. We also take the opportunity to comment on the role of the two sets of Rindler modes in the calculation presented in [1]. |
| title | Reply to 'Comment on "Ideal clocks -- a convenient fiction'' ' |
| topic | General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2604.06292 |