Building the Universe: Cold Dark Matter Theory Quiz

  • 11th Grade
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| Questions: 20 | Updated: Feb 20, 2026
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1. What does the term "cold" signify in the Cold Dark Matter (CDM) theory?

Explanation

In this context, cold means that the particles move slowly compared to the speed of light. Because they are non-relativistic, they can easily clump together under the influence of gravity. This slow motion allowed for the formation of small-scale structures in the early universe, which eventually grew into the galaxies we observe today.

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About This Quiz
Building The Universe: Cold Dark Matter Theory Quiz - Quiz

Explore the leading model for how the universe's structure formed. This Cold Dark Matter Theory Quiz examines the "slow" moving particles that clumped together under gravity to seed the birth of galaxies. Understand how this theory predicts the cosmic web and the distribution of galaxy clusters across billions of light-years.

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2. Cold Dark Matter theory suggests that large-scale structures like galaxy superclusters formed before individual galaxies.

Explanation

It is false because CDM theory follows a "bottom-up" model of structure formation. Small fluctuations in density allowed smaller objects, like sub-galactic clumps, to form first. These smaller entities then merged over billions of years to create larger structures, such as galaxies and massive clusters, driven by the gravitational pull of slow-moving dark matter.

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3. CDM particles are hypothesized to be ________, meaning they rarely interact with normal matter except through gravity.

Explanation

CDM particles are described as collisionless. This means they do not experience the electromagnetic forces that cause normal atoms to bounce off one another or emit heat. They can pass through stars, planets, and even other dark matter particles, interacting almost exclusively through gravitational attraction, which simplifies how they cluster in space.

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4. Which theoretical particle is a leading candidate for Cold Dark Matter?

Explanation

WIMPs are the primary candidates for CDM. These hypothetical particles have significant mass but only interact through gravity and the weak nuclear force. Their existence would perfectly explain the "missing mass" in galaxies and the specific way that cosmic structures evolved from the density ripples seen in the early universe's radiation.

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5. Which observations are best explained by the Cold Dark Matter model?

Explanation

Small-scale clustering, the cosmic web, and gravitational lensing are all supported by CDM. The theory accurately predicts the "web-like" distribution of matter across the cosmos. While planetary volcanism is a geological process, the distribution of entire galaxies is dictated by the scaffolding provided by the slow-moving, invisible mass described in CDM.

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6. How does Cold Dark Matter differ from "Hot" Dark Matter in terms of particle speed?

Explanation

CDM is significantly slower than Hot Dark Matter. Hot Dark Matter consists of lightweight particles, like neutrinos, that move at relativistic speeds. Because Hot Dark Matter moves so fast, it would "stream" out of small regions, preventing small galaxies from forming early on. CDM’s slower speed allows for the dense clumping observed in our universe.

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7. The Cold Dark Matter model is a key component of the Standard Model of Cosmology, often called Lambda-CDM.

Explanation

It is true because the Lambda-CDM model is the most widely accepted mathematical framework for the universe. "Lambda" represents dark energy, while "CDM" represents Cold Dark Matter. Together, these components explain how the universe expanded and how matter organized itself into the complex patterns of galaxies and voids we see through modern telescopes.

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8. In CDM theory, the universe is crisscrossed by ________ made of dark matter that connect galaxy clusters.

Explanation

The universe is crisscrossed by filaments. These are long, thin strands of dark matter that act as the skeleton of the universe. Normal baryonic matter is drawn into these filaments by gravity, leading to the formation of galaxies along these paths, creating a structure often compared to a giant cosmic spiderweb.

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9. What would happen to the formation of stars if dark matter were "hot" instead of "cold"?

Explanation

If dark matter were hot, small galaxies would not have formed early in cosmic history. Fast-moving particles would have stayed spread out, only allowing the very largest structures to collapse. Since we observe many small, old galaxies, the Cold Dark Matter theory is much better supported by our actual astronomical observations of the deep sky.

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10. Why is it difficult to detect CDM particles in a laboratory setting?

Explanation

It is difficult because they do not emit light and rarely interact with atoms. Laboratory detectors look for the tiny "kick" an atom receives when a dark matter particle hits it. Because these interactions are extremely rare and involve no electromagnetic signals, scientists must build detectors deep underground to block out other types of interference.

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11. The ________ fluctuations in the Cosmic Microwave Background provide the initial "blueprints" for CDM clumping.

Explanation

Temperature fluctuations provide the blueprints. These tiny differences in the heat of the early universe represent areas that were slightly more dense than others. Cold Dark Matter began clumping in these dense spots immediately, creating the gravitational wells that eventually pulled in enough gas to ignite the very first stars.

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12. Which force is primarily responsible for the "clumping" of Cold Dark Matter?

Explanation

Gravity is the primary force. Unlike normal matter, which is pushed around by light pressure and heat, Cold Dark Matter only feels gravity. This allows it to start forming structures much earlier than normal matter could, effectively winning the "race" to build the foundations of the galaxies that we live in today.

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13. Cold Dark Matter particles can lose energy by emitting radiation, allowing them to settle into the centers of planets.

Explanation

It is false because CDM particles cannot emit radiation. To settle into a small, dense object like a planet, matter must be able to shed energy and cool down. Since CDM does not interact with light, it cannot cool off, which is why it remains in large, diffuse halos around galaxies rather than forming solid objects.

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14. What evidence do galaxy rotation curves provide specifically for the CDM model?

Explanation

They provide evidence that mass is extended far into space. The flat rotation curves show that there is a massive amount of invisible matter extending well beyond the visible stars. This matches the CDM prediction of a large "halo" that provides the gravity necessary to keep distant stars orbiting at high speeds.

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15. What are the main ingredients of the Lambda-CDM model?

Explanation

The ingredients are Dark Energy, Cold Dark Matter, and Normal Matter. This "cosmic recipe" accounts for the expansion rate of the universe (Dark Energy), the gravitational structure (CDM), and the visible stars and planets (Baryonic Matter). This combination is currently the most successful model for describing the evolution of the cosmos from the Big Bang.

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16. CDM theory predicts that every large galaxy should be surrounded by many smaller ________ galaxies.

Explanation

The theory predicts many satellite galaxies. Because CDM forms structures from the bottom up, larger galaxies should be surrounded by smaller clumps of dark matter and stars. While we see many of these satellites around the Milky Way, the "missing satellite problem" is an area where scientists continue to refine the CDM model.

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17. How does CDM affect the path of light traveling from distant quasars?

Explanation

CDM bends the light via gravity. Even though we cannot see the dark matter itself, its mass warps the space around it. When light from a distant quasar passes through a dark matter concentration, it follows that warped path, creating multiple images or distorted arcs that scientists use to calculate the amount of CDM present.

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18. The "Dark" in Cold Dark Matter refers to the fact that it is made of dark-colored dust and rocks.

Explanation

It is false because the term refers to its invisibility, not its color. Unlike dust or rocks, which can be seen when light hits them, dark matter is completely transparent. It does not reflect or block light at all, meaning it is "dark" in the sense that it is entirely undetectable by any form of electromagnetic observation.

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19. Why is the CDM model considered "bottom-up" structure formation?

Explanation

It is considered "bottom-up" because small pieces merge into larger ones. In the early universe, CDM allowed small clumps to form first. Over time, gravity pulled these small clumps together to form galaxies, and then pulled galaxies together to form clusters. This sequence is a fundamental prediction of the Cold Dark Matter theory.

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20. What is the main goal of current experiments like those in the Large Hadron Collider regarding CDM?

Explanation

The main goal is to find the particle responsible for CDM. By smashing atoms together at high speeds, scientists hope to produce WIMPs or other dark matter candidates in a controlled environment. Confirming the identity of this particle would be one of the greatest discoveries in the history of science and the US schooling system's physics curriculum.

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What does the term "cold" signify in the Cold Dark Matter...
Cold Dark Matter theory suggests that large-scale structures like...
CDM particles are hypothesized to be ________, meaning they rarely...
Which theoretical particle is a leading candidate for Cold Dark...
Which observations are best explained by the Cold Dark Matter model?
How does Cold Dark Matter differ from "Hot" Dark Matter in terms of...
The Cold Dark Matter model is a key component of the Standard Model of...
In CDM theory, the universe is crisscrossed by ________ made of dark...
What would happen to the formation of stars if dark matter were "hot"...
Why is it difficult to detect CDM particles in a laboratory setting?
The ________ fluctuations in the Cosmic Microwave Background provide...
Which force is primarily responsible for the "clumping" of Cold Dark...
Cold Dark Matter particles can lose energy by emitting radiation,...
What evidence do galaxy rotation curves provide specifically for the...
What are the main ingredients of the Lambda-CDM model?
CDM theory predicts that every large galaxy should be surrounded by...
How does CDM affect the path of light traveling from distant quasars?
The "Dark" in Cold Dark Matter refers to the fact that it is made of...
Why is the CDM model considered "bottom-up" structure formation?
What is the main goal of current experiments like those in the Large...
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