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Article
Peer-Review Record

Gauge-Invariant Perturbation Theory on the Schwarzschild Background Spacetime: Part III—Realization of Exact Solutions

by Kouji Nakamura
Reviewer 1: Anonymous
Reviewer 2:
Submission received: 25 October 2024 / Revised: 25 November 2024 / Accepted: 24 January 2025 / Published: 6 February 2025
(This article belongs to the Special Issue Universe: Feature Papers 2024 – Compact Objects)

Round 1

Reviewer 1 Report

Comments and Suggestions for Authors

As the part III of Gauge-invariant perturbation theory on the Schwarzschild background spacetime, in this manuscipt, the author introduce some explicit example for under the Schwarzschild space time. The logic and the calculation seems correct in this manuscrpt. I have the following two question to ask: 

1) Can the author show some examples of this paper and the Regge-Wheeler gauge?

2)Can this method use to study oscillation or quasinormal modes in other compact object? such as neutron stars?

If the author can answer this two question appropriate, I will recommend this manuscript to publish in Universe. 

Author Response

Dear Sir,

I am sending the response to the comments from Reviewer 1.

My response is written in the attached pdf file.

Yours,

Kouji Nakamura

Author Response File: Author Response.pdf

Reviewer 2 Report

Comments and Suggestions for Authors

See attached PDF file.

Comments for author File: Comments.pdf

Author Response

Dear Sir,

I am sending my response to the comments from Reviewer 2.

My response is described in the attached pdf file.

Yous,

Kouji Nakamura

Author Response File: Author Response.pdf

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