<?xml version="1.0" encoding="UTF-8"?>
<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel>
<title>Krishnendu De Young Jin Suh — Neckpinch</title><link>https://neckpinch.com/authors/krishnendu-de-young-jin-suh/</link><description>New arXiv papers by Krishnendu De Young Jin Suh, from Neckpinch</description>
<atom:link href="https://neckpinch.com/authors/krishnendu-de-young-jin-suh/rss.xml" rel="self" type="application/rss+xml"/><lastBuildDate>Tue, 03 Nov 2026 08:41:12 GMT</lastBuildDate>
<item><title>Characterizations of Perfect fluid spacetimes obeying f(𝓡)-gravity equipped with different gradient solitons</title><link>https://neckpinch.com/papers/2202.03254/</link><guid isPermaLink="false">arxiv:2202.03254</guid><pubDate>Mon, 07 Feb 2022 00:00:00 GMT</pubDate><description>Krishnendu De Young Jin Suh, Uday Chand De — The prime object of this article is to study the perfect fluid spacetimes obeying f(𝓡)-gravity, when η-Ricci solitons, gradient η-Ricci solitons, gradient Einstein Solitons and gradient m-quasi Einstein solitons are its metrics. At first, the existence of the η-Ricci solitons is proved by a non-trivial example. We establish conditions for which the η-Ricci solitons are expanding, steady or shrinking. Besides, in the perfect fluid spacetimes obeying f(𝓡)-gravity, when the potential vector field of η-Ricci soliton is of gradient type, we acquire a Poisson equation. Moreover, we investigate gradient η-Ricci solitons, gradient Einstein Solitons and gradient m-quasi Einstein solitons in f(𝓡)-gravity, respectively. As a result, we establish some significant theorems about dark matter era.</description><category>Ricci solitons</category><category>Almost &amp; η-Ricci solitons</category><category>Physics</category></item>
</channel></rss>