Gates explains the importance of gravitational lensing (Einstein’s telescope). She describes the technique’s use to get better images of distant galaxies and to locate concentrations of dark matter. Dark matter has mass and just like ordinary matter can be used to magnify distant objects. While dark matter is useful as a lens it can distort images and measurements if not accounted for. Thus we need to identify the distribution of dark matter in the universe. Significantly, this will allow us to get a clearer view of the cosmic microwave background. Knowing the distribution of dark matter is essential to understanding the evolution of galaxies, their clusters and their alignment throughout spacetime. In addition we will be better able to understand dark energy.
Gates begins with several chapters devoted to basic concepts. These provide a succinct review of the Standard Model and current theories about the Big Bang, the cosmic microwave background, dark matter, dark energy and the expansion of the universe. Her chapter on special and general relativity helps explains how gravitational lensing works. Massive objects and concentrations of mass warp spacetime bending light. The larger the mass the more it curves spacetime. Dark matter does not interact with light, but it does with gravity and thus while it can’t be seen, it can be identified by its gravitational influence on objects made of ordinary matter. Dark matter forms a spherical halo around galaxies and galaxy clusters. Dark matter was essential to the evolution of the galactic structures we see.
The universe contains about five times as much dark matter as regular matter, making dark matter an excellent resource for gravitational lensing. Most of a galaxy’s power as a lens comes from its dark matter component. A nearby galaxy or a galaxy cluster can act as a powerful lens to see a distant galaxy or cluster in more detail. The amount and distribution of mass is the critical factor. Knowing this allows efficient use of this mass as a lens. The lens created by a galaxy or cluster is not smooth but lumpy depending on which components lie between the viewer and object being viewed. Thus determining the distribution of dark matter is critical but problematic since we can’t see it.
The base case for the existence of dark matter is that without it there is not enough mass in galaxies to explain their rotation speeds, their stability and even their formation. A number of theories have been considered to explain this missing mass. Some theories look to undiscovered ordinary matter such as faint stars and planets that we haven’t detected. But by and large scientists do not believe it possible for undetected ordinary matter to account for the tremendous amount of missing mass. The leading theory is that the missing mass is accounted for by an undetected particle or particles that just barely interact with regular matter except through gravity. These theorized particles are called WIMPs (Weakly interacting Massive Particles). Other hypothetical particles such as axions are also theorized to make up dark matter. However attempts to find these particles in experiments including the Large Hadron Collider have been futile. A third avenue of thought is that something is wrong with our understanding of gravity and that general relativity needs some kind of an adjustment, obviating the need to find missing matter.
Gates discusses how gravitational lensing proves dark matter exists. By looking at distant stars and galaxies that lie behind nearer galaxies and galaxy clusters in a systematic way we can identify the amount of mass in the nearby galaxy or cluster based on its magnification effects on the distant object. After thousands, even millions of observations are produced, the distribution of mass is revealed in the nearby galaxy/cluster that is used as a lens. These studies document the spherical halo of dark matter that surrounds galaxies and clusters.
Particularly significant is a collision of two galaxy clusters that occurred one hundred million years ago. We see the stars of what is known as the Bullet cluster shoot through another cluster but its galactic gas is held back by the gas of the colliding cluster and separated from the stars, planets and other objects in the Bullet cluster. Gas comprises ninety per cent of the normal matter in a galaxy, yet gravitational lensing shows most of the Bullet cluster’s mass is where its objects are, not where the gas it left behind is. Dark matter does not interact with itself and thus it kept moving along with the galaxy’s objects. Dark matter uniquely explains this disparity of mass between the Bullet cluster’s objects and gas.
Perhaps more mysterious than dark matter is dark energy. Scientists believe that space itself is expanding overcoming gravity and separating galaxy clusters from each other at an ever increasing rate. The mass in galaxy clusters still have enough gravitational force to hold together, at least for now. Competing theories for what constitutes dark energy abound including: 1) The vacuum energy of space, a constant force referenced by Einstein’s cosmological constant, 2) Quintessence in which dark energy is variable over time, and 3) Modifications to general relativity that accommodate expansion with no extra source of energy required. Of course, the answer could be a bit of all three ideas. Nobody knows.
Understanding more about dark energy means we need a better picture of the amount and distribution of matter in the universe. This means identifying the cosmic structure of dark matter through time, creating a 3D image representing billions of light years. Gravitational lensing is an essential part of doing this. Depicting the web of dark matter pervading the universe would also identify the distortions it creates and enable us to get a clearer picture of the cosmic microwave background (CMB). That might enable us to identify ancient gravity waves in the CMB emanating from the Big Bang and help us validate the theory of inflation and its various models.
Gates’ presentation is straightforward and well structured. This brief review leaves out the many supporting details that give credence to her views. These details and the methodical way she builds her case make the book engaging. The text is enhanced by many helpful pictures and illustrations. Gates succeeds in showing that gravitational lensing is essential to map the distribution of dark matter in the universe. She provides an accessible explanation of why this knowledge is needed if we are to understand the evolution and future of the universe.