
The universe contains far more than just observable matter; astronomers have discovered that a large portion of the universe is filled with two mysterious components—dark matter and dark energy—that cannot be directly observed but whose existence is inferred from gravitational effects.
Dark matter is a type of matter that does not emit or absorb light, making it undetectable through direct observation. Its existence has been proven through observations such as the unexpectedly fast rotation of galaxies, the gravitational binding of galaxy clusters, and gravitational lensing on cosmological scales.
The amount of observable matter is not sufficient to provide the gravitational force needed for galaxies and galaxy clusters to stay together. Dark matter supplies the missing gravitational force, helping to hold the structure of the universe together.
Properties of dark matter: Dark matter interacts weakly with normal matter and, being insensitive to electromagnetic forces, it neither emits nor absorbs light, making it undetectable through direct observation.
Candidates for dark matter: Scientists have developed various theories about what particles could make up dark matter. Research continues on candidates such as WIMPs (Weakly Interacting Massive Particles), axions, and MACHOs (Massive Compact Halo Objects).
Dark energy is a form of energy believed to be responsible for the accelerated expansion of the universe. It behaves as if it is spread throughout all of space, creating negative pressure that accelerates the expansion of space.
While the expansion of the universe was expected to slow down over time, observations have shown that the universe is instead expanding at an accelerating rate. The concept of dark energy was introduced to explain this acceleration.
Properties of dark energy: Dark energy is a form of energy that is homogeneously distributed throughout the universe, creating negative pressure. Its nature is not yet fully understood.
Models of dark energy: Various models for dark energy have been proposed, including the cosmological constant, scalar fields, and modified gravity theories.
The energy content of the universe is approximately 68.3% dark energy, 26.8% dark matter, and only 4.9% normal matter. This shows that a large portion of the universe is dominated by these two components, which cannot be directly observed.
In conclusion, dark matter and dark energy are among the greatest mysteries of the universe. Understanding the nature of these mysterious components will help us gain a deeper insight into the formation, evolution, and ultimate fate of the universe. Scientists continue to conduct new experiments and observations to learn more about them.
CERN. "Dark Matter." CERN Official Website. Accessed: January 3, 2025. https://home.cern/science/physics/dark-matter
CFA Harvard. "Dark Energy and Dark Matter." Harvard University Official Website. Accessed: January 3, 2025. https://www.cfa.harvard.edu/research/topic/dark-energy-and-dark-matter
Evrim Ağacı. "The 'Dark' Side of the Universe: What are Dark Matter and Dark Energy?" Evrim Ağacı Website. Accessed: January 3, 2025. https://evrimagaci.org/evrenin-karanlik-yuzu-karanlik-madde-ve-karanlik-enerji-nedir-8420?srsltid=AfmBOorTC8DPVGf89gtMZ6Q9ITM-ID1vE65R4ii1okrSYbU2PKDOTqKr

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