Reply to the comments of Karami on the Interacting holographic dark energy model and generalized second law of thermodynamics in a non-flat universe

TL;DR

This paper addresses and corrects a calculation error in a previous work on holographic dark energy and thermodynamics in a non-flat universe, reaffirming the validity of the original results under certain parameter conditions.

Contribution

It clarifies and corrects a calculation error pointed out in a comment, confirming the original model's validity for specific parameter values.

Findings

The original results are valid if the free parameter b^2 > 0.264.

The calculation error was trivial and does not affect the main conclusions.

The discussion remains consistent within the specified parameter range.

Abstract

In [arXiv:0911.4808] K. Karami commented on my publication [arXiv:hep-th/0701242] and claimed that my result would be invalid. In fact he found an error in calculation of the entropy of cold dark matter in section 3 of my article, which is, however, a rather trivial one. It is shown that my discussion in section 3 of my paper works correctly if we take the value of free parameter $b^2>0.264$.