Dark Matter, Dark Energy: The Dark Side of the Universe

Course No. 1272
Professor Sean Carroll, Ph.D.
California Institute of Technology
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Course No. 1272
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What Will You Learn?

  • numbers Survey the visible universe, from the known stars in our galaxy to fascinating nebulae.
  • numbers Peer into atoms to discover the nuclei and electrons that constitute ordinary matter.
  • numbers Learn about a bold new field in nature known as quintessence.

Course Overview

There's more to the universe than meets the eye—a lot more. In recent years, scientists have discovered that 95% of the contents of the cosmos are invisible to our current methods of direct detection. Yet something is holding galaxies and galaxy clusters together, and something else is causing space to fly apart.

Scientists call these invisible components dark matter and dark energy; "dark" because these phenomena do not emit light, not because we are not learning more and more about them. In fact, dark matter and dark energy are the most eagerly studied subjects in astronomy and particle physics today.

If and when we discover this matter, it will further validate the "standard model" of physics which, so far, is the best description of how our universe works; if we cannot find this matter, or if it does not exist, then we will completely need to rethink the current "standard model" theory.

Join the exciting search for these mysterious phenomena in Dark Matter, Dark Energy: The Dark Side of the Universe, a mind-expanding, 24-lecture course taught by Dr. Sean Carroll, a theoretical physicist with a profound knowledge of the field. Starting with the early 20th-century work of Albert Einstein in theoretical physics and Edwin Hubble in observational astronomy, Dr. Carroll takes you through the key concepts of this revolutionary view of an expanding universe, concepts which have brought us—for the first time in history—to the brink of knowing what the universe is made of.

Welcome to the Dark Side

Everything you see with your eyes and with powerful instruments—stars, planets, galaxies, dust, and gas—and everything that you think of as atom-based matter is only 5% of what we now know exists. The rest is what Dr. Carroll calls the "dark sector," which consists of the following:

  • Dark matter: First proposed in the 1930s, the idea that there is missing mass influencing the behavior of galaxies began to look more and more likely from the 1970s on. We know that it is matter because we can detect its gravitational influence on visible matter, but we cannot see it. An inventory of the distribution of dark matter throughout space shows that it constitutes 25% of the energy density of the universe.
  • Dark energy: The greatest discoveries are the unexpected ones, which was the case in the late 1990s when two teams of astronomers competing to measure the rate at which the expansion of the universe is slowing down (as virtually everyone thought it must be) discovered that it is speeding up instead. A previously unknown, all-pervasive dark energy must be at work, representing 70% of the energy density of the universe.

Together, dark matter and dark energy account for all but a tiny fraction of everything there is; the ordinary matter that is left over is like the seasoning on the main dish. The story of how we arrived at this startling cosmic recipe is an absorbing drama that takes you through the breakthrough discoveries in astronomy and physics since the turn of the 20th century.

Concept by concept, Dark Matter, Dark Energy gives you the tools to appreciate this subject in depth. Dr. Carroll explains why scientists believe we live in a smooth, expanding universe that originated in a hot, dense state called the big bang.

You investigate the features of the infant universe that led to the large-scale structure we observe today, explore the standard model of particle physics and see how it provides the framework for understanding the interaction of all matter and radiation, and come to understand why dark matter and dark energy are logical consequences of a range of scientific theories and observations and how together they complete a grand picture of the universe.

Deduce the Existence of the Dark Sector

Several significant clues disclose the existence of dark matter and dark energy. In the case of dark matter, we have the evidence of:

  • Galaxy dynamics: The motions of the stars in galaxies and galaxies within clusters indicate that there is far more matter than is implied by visible stars and gas.
  • Echoes of the big bang: Variations in the leftover radiation from the big bang demonstrate that there must be dark matter pulling the ordinary matter we see.

Dark matter is clear to see compared to dark energy, which reveals itself subtly but unmistakably through:

  • Exploding stars: Type Ia supernovae provide a standard candle to measure the distances to faraway galaxies. By combining this information with redshift (which measures how fast a galaxy recedes), astronomers conclude that something is causing galaxies to recede at a faster and faster velocity.
  • Geometry of space: Observations that space is "flat" (with neither positive nor negative curvature) imply a total energy density for the universe that is stunningly consistent with the dark energy hypothesis.

Each of these techniques deduces the existence of dark matter or dark energy from the gravitational fields they cause. But what if our theory of gravity is faulty? Could adjustments to Einstein's general theory of relativity, which forms our modern understanding of gravity, do away with the need for the dark sector?

You explore a theory called Modified Newtonian Dynamics, which successfully dispenses with dark matter in individual galaxies. This theory fails, however, when applied to clusters and has nothing to say about the expansion of the universe.

"It is impossible, in principle, to think of a theory in this day and age that will completely do away with dark matter," says Dr. Carroll, pointing in particular to a convincing piece of evidence from the aftermath of the collision of two galaxies.

Known as the Bullet Cluster, it shows a central region of ordinary matter (evident through telltale x-ray emissions), on either side of which are far more extensive clouds of what can only be dark matter, disclosed by gravitational lensing.

Explaining away dark energy is similarly difficult, because it requires revising the fundamental equation of general relativity. "The problem is that this equation of Einstein's is actually quite remarkable," says Dr. Carroll. "If you try to mess with it just a little bit, you break it."

The overriding question remains: What are dark matter and dark energy? We do not yet know for certain, but physicists have come up with an array of creative ideas and ways to test them. Dark Matter, Dark Energy covers the most promising proposals and looks ahead to experiments that will dramatically improve our understanding of the dark sector.

Take a Voyage of Scientific Discovery

Dr. Carroll has a knack for explaining the latest complex picture of the universe in easy-to-follow terms—a skill honed by his more than 250 scientific seminars, colloquia, educational discussions, and popular talks. Relaxed, eloquent, wryly funny, and brimming with ideas, he has received the Graduate Student Council Teaching Award from MIT for his course on general relativity, as well as research grants from NASA, the U.S. Department of Energy, and the National Science Foundation.

With his expert guidance, your previously held ideas about the fate (and possibly the origin) of the universe will be altered permanently. A rich voyage of scientific discovery, Dark Matter, Dark Energy provides you with a comprehensive look at these two mysterious phenomena—and their startling implications for our understanding of the universe.

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24 lectures
 |  Average 31 minutes each
  • 1
    Fundamental Building Blocks
    Scientists now have a complete inventory of the universe, which is composed of three basic constituents: Ordinary matter includes every kind of particle ever directly observed; dark matter consists of massive particles known only because of their gravitational effects; and dark energy is a smoothly distributed component that whose density does not change as the universe expands. x
  • 2
    The Smooth, Expanding Universe
    Imagine looking into a clear night sky with perfect vision. What would you see? This lecture surveys the visible universe—from the stars in our galaxy to the cloudy patches called nebulae that astronomer Edwin Hubble proved are galaxies in their own right—and Hubble's discovery that the universe is expanding. x
  • 3
    Space, Time, and Gravity
    Einstein taught us that space and time can be combined into spacetime, which has the ability to evolve and grow. Indeed, what we think of as gravity is just a manifestation of the curvature of spacetime. To find things in the universe—including dark matter and dark energy—all we have to do is to map out this curvature. x
  • 4
    Cosmology in Einstein's Universe
    The expansion of the universe is governed by its spatial curvature and energy density, both of which have specific ways of changing as the universe grows. These features are related to each other by Einstein's general theory of relativity, which can be used to model the past and possible future of the universe. x
  • 5
    Galaxies and Clusters
    Applying the laws of dynamics to galaxies and galaxy clusters, we find that more matter is required to account for their motions than can be observed. Some of the missing mass is hot gas; however, this is still not enough, and we need to invoke some new kind of particle in galaxies and clusters: dark matter. x
  • 6
    Gravitational Lensing
    Another way to detect invisible matter is to use light as a probe of the gravitational field. Passing through curved spacetime, the path of a light ray is deflected due to gravitational lensing. Lensing demonstrates the existence of gravitational fields where there is essentially no ordinary matter. x
  • 7
    Atoms and Particles
    We peer into the atom to discover the constituents of ordinary matter: nuclei and electrons. Nuclei are made of protons and neutrons, which in turn are made of quarks. Electrons and quarks are examples of fermions, or matter particles. There are also bosons, or force-carrying particles, such as photons and gluons. x
  • 8
    The Standard Model of Particle Physics
    In the 1960s and 1970s, physicists developed a comprehensive theory of known fermions and bosons. Now called the standard model, this theory fits an impressive amount of data, but it leaves two crucial puzzles: the hypothetical Higgs boson and the graviton, the carrier of the gravitational force. x
  • 9
    Relic Particles from the Big Bang
    Armed with the core principles of particle physics, we know enough about the early universe to predict how many of each type of particle should be left over from the Big Bang. These "relic abundances" are crucial to understanding the origin of dark matter and light elements. x
  • 10
    Primordial Nucleosynthesis
    The process of nucleosynthesis describes how protons and neutrons were assembled into light elements during the first few minutes after the Big Bang. We can observe these primordial elements today and check on Einsteinian cosmology and a stringent constraint on theories of dark matter. x
  • 11
    The Cosmic Microwave Background
    About 380,000 years after the Big Bang, the universe had cooled sufficiently for electrons and nuclei to combine into atoms allowing light to travel much more freely. The relic photons from this era are visible to us today as the cosmic microwave background, which holds clues to the composition and structure of the universe. x
  • 12
    Dark Stars and Black Holes
    Candidates for dark matter include small, dark stars called Massive Compact Halo Objects (MACHOs) and black holes. Such objects are ultimately composed of ordinary matter, of which there just isn't enough to account for the dark matter. We are forced to conclude that the dark matter is a new kind of particle. x
  • 13
    WIMPs and Supersymmetry
    Weakly interacting massive particles (WIMPs) are ideal candidates for what comprises dark matter. WIMPs may have their origins in supersymmetry, which posits a hidden symmetry between bosons and fermions, and predicts a host of new, as-yet-unobserved particles, including WIMPs. x
  • 14
    The Accelerating Universe
    In the late 1990s, two groups of astronomers found to their astonishment that the expansion of the universe is speeding up rather than slowing down. Such behavior can't be explained by any kind of matter and suggests the existence of an entirely new component: dark energy. x
  • 15
    The Geometry of Space
    Precise measurements of the cosmic microwave background let us measure the total energy density of the universe by observing the geometry of space. We find that the energy in matter alone is not enough, confirming the need for dark energy. x
  • 16
    Smooth Tension and Acceleration
    Dark energy is smoothly distributed throughout the universe and its density is nearly constant, even though the universe is expanding. Unlike gas under pressure in a container, dark energy is a kind of "negative pressure"—or tension—that imparts an accelerated expansion to the universe. x
  • 17
    Vacuum Energy
    The density and distribution of dark energy remain the same across all of space­time, but what exactly is dark energy? There are many possibilities, the simplest of which is vacuum energy—an constant amount of energy in every cubic centimeter of space itself. Vacuum energy is equivalent to Einstein's idea of the cosmological constant. x
  • 18
    Quintessence
    Another idea about dark energy is that it results from a new field in nature, analogous to the electromagnetic field but remaining persistent as the universe expands. This field is called quintessence. It would be observationally distinguishable from the cosmological constant. x
  • 19
    Was Einstein Right?
    We have inferred the existence of dark matter and dark energy from the gravitational fields they cause. In this lecture, we explore proposals that a modified theory of gravity might allow us to dispense with the need for invoking dark stuff. However, this turns out to be very difficult in practice. x
  • 20
    Inflation
    Before we had observational evidence that the universe is accelerating, cosmologists considered the possibility of a period of rapid acceleration at very early times—a scenario known as inflation. x
  • 21
    Strings and Extra Dimensions
    We know about the dark sector because of gravity, and string theory is an ambitious attempt to unify gravitation with the other forces of nature into a theory of everything. String theory promises a theory of quantum gravity, but it also predicts extra, unseen spatial dimensions that are difficult to test. x
  • 22
    Beyond the Observable Universe
    The speed of light and the age of the observable universe are finite. That means we can't see the whole universe because our vision can only stretch so far. The "multi­verse"—a hypothesis of regions where conditions are very different from those we see in our observable universe—may help explain properties of dark energy. x
  • 23
    Future Experiments
    Astronomers are designing new observatories to probe the acceleration of the universe and other cosmic phenomena. Physicists are also looking forward to new experiments that will dramatically improve our understanding of particles and forces, and how ordinary matter fits in with dark matter and dark energy. x
  • 24
    The Past and Future of the Dark Side
    The concordance cosmology is an excellent fit to a variety of data, but it presents us with deep puzzles: What are dark matter and dark energy? Why do they have the densities they do? Our own universe seems unnatural to us. That's good news, as it is a clue to the next level of understanding. x

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Your professor

Sean Carroll

About Your Professor

Sean Carroll, Ph.D.
California Institute of Technology
Professor Sean Carroll is a Senior Research Associate in Physics at the California Institute of Technology. He earned his undergraduate degree from Villanova University and his Ph.D. in Astrophysics from Harvard in 1993. Before arriving at Caltech, Professor Carroll taught in the Physics Department and the Enrico Fermi Institute at the University of Chicago, and did postdoctoral research at the Massachusetts Institute of...
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Reviews

Dark Matter, Dark Energy: The Dark Side of the Universe is rated 4.7 out of 5 by 152.
Rated 5 out of 5 by from Awesome Course! Only half way through and really like this course! The written material from the download saves me time from taking notes. The instructor has an awesome way of explaining complex facts. I will be reviewing it again to further my understanding.
Date published: 2020-11-12
Rated 5 out of 5 by from Can not wait for a sequel Excellent course, each lecture is interesting and very entertaining
Date published: 2020-08-12
Rated 5 out of 5 by from What we can't see can inform us This is an excellent course. It was made prior to the Planck spacecraft launch and discovery of the Higgs boson, but both are mentioned. Doctor Carroll is a remarkably good instructor who not only tells us where we are and where we are headed, but also why the destination is important and the questions we should ask along the way. Finally, take heart those with limited math skills. If you can add 5%, 25%, and 70% and get 100%, you are mathematically qualified to understand this course.
Date published: 2020-08-03
Rated 5 out of 5 by from Very understandable The lectures are just the right length and not boring! Explanations are in language a non-astronamer, like myself can understand. Just wish I could figure out how to get closed captioning along with the lectures.
Date published: 2020-06-17
Rated 5 out of 5 by from Professionally presented!! Sean Carroll is one of the most engaged and knowledgeable teacher of difficult subjects in science: particle physics. It was a delight to learn this subject. It will be sensible to watch again because of my interest in such material.
Date published: 2020-04-29
Rated 3 out of 5 by from Out of date This was done in 2007. There have been a lot of new discoveries since then. The Higgs boson was seen. Gravity waves were detected. New questions have arisen. This course to too outdated to be offered. The presentation was very well done though.
Date published: 2020-02-04
Rated 5 out of 5 by from informative A course presenting a very complex subject in easy to understand lecture by a very talented lecturer.
Date published: 2019-05-18
Rated 5 out of 5 by from Outstanding presentation and explanation ! Dr. Sean Carroll presents concepts in astrophysics and particle physics in very clear and understandable format. I would highly recommend this course to anyone who is interested in the wonders of the universe in which we live.
Date published: 2019-04-15
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