Dark Matter Explained - And Why It Might NOT Exist!

Support the Research Behind this Channel on Patreon: https://www.patreon.com/arvinash REFERENCES Strongest Evidence favoring Dark Matter https://youtu.be/HRMR7eMKLz0 Strongest Evidence AGAINST Dark Matter https://youtu.be/zZYHPSONxqI How to "Catch" Dark Matter https://youtu.be/ufZ5_bc6aqM Strongest Candidates for the Dark Matter "Particle" https://youtu.be/915Vky7r_gk CMB Simulator https://plancksatellite.org.uk/cmb-sim/ CHAPTERS 0:00 Missing Gravity Problem of Cosmos 0:45 How Dark Matter was theorized 2:44 How do we know Dark Matter affected the early universe? 5:48 How do we "see" Dark Matter, even though it's invisible? 7:48 How can we be so sure that dark matter exists? 11:02 What could the dark matter "particle" be? WIMP 12:22 Neutralinos & Why Dark Matter must interact with the Weak Nuclear force? 14:04 Second viable candidate for Dark Matter: Axion 17:22 The case AGAINST Dark Matter - the story 18:48 Modified Newtonian Dynamics (MOND) 12:20 Why don't we get rid of Dark Matter? SUMMARY This video summarizes the mystery of dark matter, the unseen substance believed to make up most of the matter in the universe. Although the cosmos appears full of luminous objects such as stars, galaxies, and glowing gas, scientists have discovered that the majority of matter does not emit, absorb or reflect light. This invisible component is called dark matter. The video aims to explain what dark matter is, the evidence suggesting it exists, possible explanations for what it might be made of, and why some scientists question whether it exists at all. Dark matter is defined as a form of matter that does not interact with light or any other type of electromagnetic radiation. Because it neither emits nor reflects light, it cannot be observed directly with telescopes. Instead, astronomers infer its existence through its gravitational influence on visible matter and the structure of the universe. Current estimates suggest that dark matter makes up roughly 85% of all matter in the universe, leaving ordinary matter—atoms that form stars, planets, and people—as only a small fraction of the total. The strongest evidence for dark matter comes from astronomical observations, particularly the rotation of galaxies. According to Newtonian gravity and the visible mass within galaxies, stars located far from a galaxy’s center should move more slowly than those near the center. However, observations show that outer stars move much faster than expected. If only visible matter were present, galaxies would not remain stable—they would fly apart. The most widely accepted explanation is that galaxies are embedded in halos of unseen mass that provide additional gravitational pull. This hidden mass is what scientists call dark matter. Because dark matter cannot be made of ordinary atoms—since normal matter interacts with light—physicists have proposed several hypothetical particle candidates. One leading possibility is WIMPs (Weakly Interacting Massive Particles), particles that interact through gravity and the weak nuclear force but rarely interact with other matter. Another candidate is the axion, a very light particle originally proposed to solve a theoretical problem in quantum chromodynamics. A third possibility involves MACHOs (Massive Compact Halo Objects) such as faint stars, black holes, or other compact objects. However, observations suggest that MACHOs cannot account for the total amount of dark matter needed to explain cosmic structures. The video also clarifies the difference between dark matter and dark energy, two concepts often confused because of their names. Dark matter acts as an additional source of gravity that helps hold galaxies together, while dark energy is a completely different phenomenon—an unknown form of energy that permeates space and drives the accelerated expansion of the universe. Despite strong observational evidence, dark matter has never been directly detected. This has led some physicists to propose alternative ideas such as Modified Newtonian Dynamics (MOND). MOND suggests that the laws of gravity may behave differently at extremely low accelerations, which could explain galaxy rotation without invoking unseen matter. While MOND successfully predicts some galactic behavior, it struggles to explain larger-scale observations such as galaxy clusters and patterns in the cosmic microwave background. #darkmatter Dark matter remains one of the most important unsolved problems in physics. Whether the solution involves new particles, new physics, or a deeper understanding of gravity, solving this mystery could fundamentally reshape our understanding of the universe.