Okay, so let’s start with the obvious. The big bang is not dead. Recent observations by the James Webb Space Telescope have not disproven the big bang, despite certain popular articles claiming otherwise. If that’s all you needed to hear, then have a great day. That said, the latest Webb observations do reveal some strange and unexpected things about the universe, and if you’d like to know more, keep reading.
Let’s start with the rumors. What about the new Webb data would suggest the big bang is wrong? The same type of data Hubble gave us years ago. We generally think of evidence for the big bang being centered around two facts: first, that more distant galaxies have a higher redshift than closer ones, and second, that the universe is filled with a cosmic background of microwave radiation. The first suggests that the universe is expanding in all directions, while the second suggests that it was once in a very hot and dense state. These are two of the Three Pillars of data supporting the big bang, the third being the relative abundance of elements in the early universe.
But these observations are just the foundation of the big bang model. We have long since expanded on these to create the standard model of cosmology, also known as the LCDM model. That is a universe that began with the big bang and is filled with matter, dark matter, and dark energy. Everything from the acceleration of cosmic expansion to the clustering of galaxies supports this standard model. And the standard model makes predictions about other observational tests, so we can further prove its validity. That’s where the latest claims of the “big bust” come into play.
One of these secondary tests is known as the Tolman surface brightness test. It was first proposed in the 1930s by Richard C. Tolman and compares the apparent brightness of a galaxy with its apparent size. The ratio of brightness to size is known as surface brightness. Generally, the bigger a galaxy, the brighter it should be, so the surface brightness of every galaxy should be roughly the same. More distant galaxies would appear dimmer, but they’d also have a smaller apparent size, so the surface brightness would still be the same. The Tolman test predicts that in a static, non-expanding universe the surface brightness of all galaxies should be about the same, regardless of distance.
This isn’t what we see. What we observe is that more distant galaxies have a dimmer surface brightness than closer ones. The amount of dimming is proportional to the amount of redshift the galaxy has. You might think this proves that all those distant galaxies are speeding away from us, but it actually doesn’t. If those distant galaxies were speeding away, you’d have two dimming effects. The red shift and the ever-increasing distance. The Tolman test predicts that in a simple expanding universe the surface brightness of galaxies should diminish proportional to both redshift and distance. We only see the effects of redshift.
This fact has led some to propose a static universe where light spontaneously loses energy over time. It’s the so-called tired light hypothesis, and it’s very popular among big bang opponents. If the universe is static and light is tired, then the Tolman test predicts exactly what we observe. Hence no big bang.
Back in 2014, Eric Lerner et al published a paper making exactly this point. It caused a flurry of “Big Bang Dead!” articles in the popular media. The latest claims about Webb killing the big bang began with a popular article by the same Eric Lerner. So here we are. In fairness, back in 2014, the Hubble observations supported Lerner’s claim, and so do the latest Webb observations. But what Lerner conveniently omitted from his paper is that the Hubble and Webb observations also support the LCDM model.
It’s a common misconception that redshift proves that galaxies are speeding away from us. They aren’t. Distant galaxies aren’t speeding through space. Space itself is expanding, putting greater distance between us. It’s a subtle difference, but it means that galactic redshift is caused by cosmic expansion, not relative motion. It also means that distant galaxies appear a bit larger than they would in a static universe. They are distant and tiny, but the expansion of space gives the illusion of them being larger. As a result, the surface brightness of distant galaxies dims only proportional to redshift.
Of course, we know tired light is wrong because of the cosmic microwave background. A static, tired-light universe wouldn’t have any remnant heat from a primordial fireball. Not to mention the fact that distant galaxies would appear blurred (they don’t), and distant supernovae wouldn’t be time-dilated by cosmic expansion (they are). The only model that supports all the evidence is the big bang. Lerner’s argument is an old one that has long been disproven.
All that said, the James Webb Space Telescope has found some unusual things. Most significantly, it has found more galaxies and more distant galaxies than there should be, and that could lead to some revolutionary changes in our standard model. Our current understanding is that after the big bang the universe went through a period known as the dark ages. During this period the first light of the cosmos had faded, and the first stars and galaxies hadn’t yet formed. Webb is so sensitive it can see some of the youngest galaxies that formed just after the dark ages. We would expect those young galaxies to be less numerous and less developed than later galaxies. But the Webb observations have found very redshifted, very young galaxies that are both common and surprisingly mature.
It’s the kind of puzzling and unexpected data astronomers were hoping for. It’s why we wanted to build the Webb telescope in the first place. And it tells us that while the big bang model isn’t wrong, some of our assumptions about it might be.
Reference: Lerner, Eric J., Renato Falomo, and Riccardo Scarpa. “UV Surface Brightness of Galaxies from the Local Universe to z~ 5.” International Journal of Modern Physics D 23.06 (2014): 1450058.
Reference: Ferreira, Leonardo, et al. “Panic! At the Disks: First Rest-frame Optical Observations of Galaxy Structure at z > 3 with JWST in the SMACS 0723 Field.” arXiv preprint arXiv:2207.09428 (2022).
Good reporting and explanation. Coincidentally, I met Eric Lerner several years ago. He came to my work (I’m not going to elaborate about where I work) to give us a presentation about his pinched fusion concept. He was looking for funding to continue his fusion research. I did not realize that he also wrote these types of articles, but good to know.
It’s a bit unclear from the article, but Wikipedia clarifies:
“To date, the best investigation of the relationship between surface brightness and redshift was carried out using the 10 m Keck telescope to measure nearly a thousand galaxies’ redshifts and the 2.4 m Hubble Space Telescope to measure those galaxies’ surface brightness.[1] The exponent found is not 4 as expected in the simplest expanding model, but 2.6 or 3.4, depending on the frequency band. The authors summarize:
“We show that this is precisely the range expected from the evolutionary models of Bruzual & Charlot. We conclude that the Tolman surface brightness test is consistent with the reality of the expansion.””
Looking in Sandage et al. paper [arXiv:astro-ph/0106566] it seems it is the luminosity evolution which has to be accounted for. Doing that rejects “tired light” ideas, which i guess Lerner et al. somehow forget to mention:
“The resulting exponents are too large by approximately 5 and 10 ?, respectively, compared to the n = 1 prediction of the “tired light” scenario. Consequently, to produce coherence with the “tired light” model, we require negative luminosity evolution in the look-back time, i.e. galaxies must be fainter in the past. No feasible model of stellar evolution can produce such luminosity evolution with time.”
To pile on, the day after this article NASA posted a shoot out to their co-authorship in a DES publication [arXiv:2207.05766] that shows LCDM is the best model still.
“A new study from the international Dark Energy Survey, using the Victor M. Blanco 4-meter Telescope in Chile, marks the latest effort to determine whether this is all simply a misunderstanding: that expectations for how gravity works at the scale of the entire universe are flawed or incomplete. This potential misunderstanding might help scientists explain dark energy. But the study – one of the most precise tests yet of Albert Einstein’s theory of gravity at cosmic scales – finds that the current understanding still appears to be correct.”
[“NASA Scientists Help Probe Dark Energy by Testing Gravity”]
The paper tests a lot of various extensions and then ends:
“In summary, we achieve precise and robust tests of extensions to ?CDM thanks to the powerful DES Y3 3×2pt measurements in combination with other state-of-the-art cosmological data, while underlining challenges that will need to be addressed for future wide field galaxy surveys to further test the laws and contents of the Universe. We ultimately detect no significant preference for any of the extended models studied in our analysis. Thus, ?CDM remains the favored model to describe our data.”