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In this manuscript, we consider the Schwarzschild black hole surrounded by
the quintessence matter in noncommutative spacetime. At first, we examine its
thermodynamics in the context of the Hawking temperature, entropy, and specific
heat functions. Then, we discuss the phase transitions and stability. Next, we
predict the shadow images in the presence of plasma. After visualizing these
results, we derive the quasinormal modes in WKB and Mashhoon approximations.
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