Acoustic black hole in noncommutative space: Solutions and thermodynamical analysis

The inability of sound disturbances to escape from a fluid moving faster than sound is known as an acoustic black hole. These black holes either create or encourage this radiation, which is called phono-Hawking. On the other hand, the event horizon is a sound black hole’s boundary. Our goal is to use the spatial–spatial quatification provided by inspired noncommutativity to observe the quantum influence on sonor black hole features. The stuff characterizing the fluid is affected by such a distortion.