2023
DOI: 10.55730/1300-0098.3423
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Perfect fluid spacetimes and $k$-almost Yamabe solitons

Abstract: In this article, we presumed that a perfect fluid is the source of the gravitational field while analyzing the solutions to the Einstein field equations. With this new and creative approach, here we study k-almost yamabe solitons and gradient k-almost yamabe solitons. First, two examples are constructed to ensure the existence of gradient k-almost Yamabe solitons. Then we show that if a perfect fluid spacetime admits a k-almost yamabe soliton, then its potential vector field is Killing if and only if the diver… Show more

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Cited by 6 publications
(5 citation statements)
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“…Because of their connection to GR, there was a notable increase of quest in researching Ricci solitons and related generalizations in a variety of geometrical contexts. Many researchers have investigated many sorts of solitons in P F spacetimes including Ricci and gradient type Ricci solitons ( [17], [18]), η-Ricci solitons [4], Yamabe and gradient type Yamabe solitons [17], k-almost Yamabe solitons [15], η-Einstein solitons of gradient type [18], gradient ϱ-Einstein solitons [13], m-quasi Einstein solitons of gradient type [17], gradient Schouten solitons [18], Ricci-Yamabe solitons [14], respectively.…”
Section: Theorem C([25])mentioning
confidence: 99%
“…Because of their connection to GR, there was a notable increase of quest in researching Ricci solitons and related generalizations in a variety of geometrical contexts. Many researchers have investigated many sorts of solitons in P F spacetimes including Ricci and gradient type Ricci solitons ( [17], [18]), η-Ricci solitons [4], Yamabe and gradient type Yamabe solitons [17], k-almost Yamabe solitons [15], η-Einstein solitons of gradient type [18], gradient ϱ-Einstein solitons [13], m-quasi Einstein solitons of gradient type [17], gradient Schouten solitons [18], Ricci-Yamabe solitons [14], respectively.…”
Section: Theorem C([25])mentioning
confidence: 99%
“…They obtained a number of interesting results and inspired the idea of this paper. De and Gezer [32] studied k-almost Yamabe solitons for the perfect fluid spacetime of general relativity. In particular, they constructed two examples to prove the existence of k-almost Yamabe solitons.…”
Section: Introductionmentioning
confidence: 99%
“…Bracken and Azami obtained some results on the evolution of the first eigenvalue recently [4][5][6]. Other remarkable work can be found in [7][8][9][10]. We call the smooth function u : M → R a harmonic function if ∆u = 0.…”
Section: Introductionmentioning
confidence: 99%