For more detail on the unification of space and time, see pp. 73–79 of Black Holes & Time Warps (Thorne 1994). For the superstring breakthrough by John Schwarz and Michael Green and how that forced physicists to embrace a bulk with extra dimensions, see The Elegant Universe: Superstrings, Hidden Dimensions, and the Quest for the Ultimate Theory (Greene 2003).
For a highly rated, animated movie of Edwin A. Abbott’s Flatland (Abbott 1884), see Flatland: The Film (Ehlinger 2007). For extensive discussions of the mathematics underlying Flatland and the story’s connections to nineteenth-century English society, see The Annotated Flatland: A Romance of Many Dimensions (Stewart 2002). For visual insights into the fourth space dimension, see The Visual Guide to Extra Dimensions, Volume 1: Visualizing the Fourth Dimension, Higher-Dimensional Polytopes, and Curved Hypersurfaces (McMullen 2008).
For much of the content of this chapter, I recommend Warped Passages: Unraveling the Mysteries of the Universe’s Hidden Dimensions (Randall 2006). This is a thorough discussion of modern physicists’ ideas and predictions about the bulk and its extra dimensions, written by Lisa Randall who, with Raman Sundrum, discovered that AdS warping can confine gravity near our brane (Figures 23.4 and 23.6). The idea of an AdS layer and sandwich, which I rediscovered, was first proposed and discussed in a technical paper by Ruth Gregory, Valery A. Rubakov, and Sergei M. Sibiryakov (Gregory, Rubakov, and Sibiryakov 2000), and the AdS sandwich was shown to be unstable in a technical paper by Edward Witten (Witten 2000).
For the history of the anomalous precession of Mercury’s orbit and the search for the planet Vulcan, I recommend a scholarly treatise by science historian N. T. Roseveare, Mercury’s Perihelion from Le Verriere to Einstein (Roseveare 1982), and also the more readable but less comprehensive account by astronomers Richard Baum and William Sheehan, In Search of the Planet Vulcan: The Ghost in Newton’s Clockwork Universe (Baum and Sheehan 1997).
For the discovery of evidence for dark matter in our universe and the current search for dark matter, I recommend a highly readable book, The Cosmic Cocktaiclass="underline" Three Parts Dark Matter (Freeze 2014), by one of the leading researchers in this quest, Katherine Freeze.
For the anomalous acceleration of the universe’s expansion and the dark energy that presumably causes it, I recommend the last chapter of The Cosmic Cocktail (Freeze 2014) and also The 4% Universe: Dark Matter, Dark Energy, and the Race to Discover the Rest of Reality (Panek 2011).
The ideas that Newton’s gravitational constant G might change from place to place and time to time, and might be controlled by some sort of nongravitational field, were hot topics in the Princeton University physics department when I was a PhD student there in the early 1960s. These ideas had been proposed by Princeton’s Professor Robert H. Dicke and his graduate student Carl Brans in connection with their “Brans-Dicke theory of gravity” (Chapter 8 of Was Einstein Right? [Will 1993]), an interesting alternative to Einstein’s general relativity. For a brief personal memoir about this, see “Varying Newton’s Constant: A Personal History of Scalar-Tensor Theories” in Einstein Online (Brans 2010). The Brans-Dicke theory has motivated a number of experiments that searched for varying G, but no convincing variations were ever found; see, for example, Chapter 9 of Was Einstein Right? (Will 1993). These ideas and experiments motivated my interpretation of some of Interstellar’s gravitational anomalies and how to control them: bulk fields control the strength of G and make it vary.
The Professor’s equation, shown on his blackboard in Figure 25.6, builds on these ideas. It also incorporates Einstein’s relativistic laws (general relativity), extended into the bulk’s fifth dimension, which are laid out in a technical review article by Roy Maartens and Koyama Kazuya (Maartens and Kazuya 2010), and it incorporates a branch of mathematics called the “calculus of variations”; see, for example, http://en.wikipedia.org/wiki/Calculus_of_variations. For a few technical details about the Professor’s equation, see the appendix Some Technical Notes.
For a first foray into quantum fluctuations and quantum physics more generally, I recommend The Ghost in the Atom: A Discussion of the Mysteries of Quantum Physics (Davies and Brown 1986). I don’t know any articles or books for nonphysicists about the quantum behavior of human-sized objects such as LIGO’s mirrors; at a technical level, I discuss this in the second half of my third Pauli lecture (the one listed first) at http://www.multimedia.ethz.ch/speakers/pauli/2011. In John Wheeler’s autobiography, he discusses how he came up with the idea of quantum foam (Chapter 11 of Geons, Black Holes and Quantum Foam: A Life in Physics [Wheeler and Ford 1998]).
In Chapter 11 of Black Holes & Time Warps (Thorne 1994) I discuss what was known in 1994 about the interiors of black holes, and how we came to know it—including the BKL singularity and its dynamics; quantum gravity’s control of the singularity’s core and its connection to quantum foam; and the infalling singularity (mass-inflation singularity), which had only recently been discovered by Erik Poisson and Werner Israel (Poisson and Israel 1990) and was not yet fully understood. The upflying singularity was discovered so recently that there is not yet any detailed discussion of it for nonphysicists; the technical discovery article is Marolf and Ori (2013) by Donald Marolf and Amos Ori. Matthew Choptuik’s discovery that tiny, transient naked singularities are possible was announced and explained in his technical article (Choptuik 1993).
The volcano-like surface that underlies much of this chapter (Figures 27.3, 27.5, and 27.9) can be described with elementary physics equations, as can the Endurance’s trajectory, the trajectory’s instability on the rim, and the Endurance’s launch toward Miller’s planet. See the appendix Some Technical Notes.
In the Prologue of Black Holes & Time Warps (Thorne 1994), I describe, in much greater detail than here, what it would look like and feel like to fall through a black hole’s horizon, both as seen and felt by the infalling person and as seen by someone else outside the black hole. And I describe how the look and feel are influenced by the mass of the black hole and by its spin.
Andrew Hamilton has constructed a “Black Hole Flight Simulator” for computing what it looks like to fall into a nonspinning black hole. His computations are similar to those done for Interstellar by Paul Franklin’s team (Chapters 8, 9, and 15), but preceded Interstellar by many years. Andrew has used his simulator to produce a remarkable set of film clips that can be found on his website, http://jila.colorado.edu/~ajsh/insidebh, and in planetariums around the world (see http://www.spitzinc.com/fulldome_shows/show_blackholes).