How Theories Are Born, Live, and Die
The rise and fall of citations reveals how concepts gain acceptance and fade away.
Imagine if you could track the lifespan of an idea—see it born, watch it grow, witness its golden years, and eventually see it fade away to make room for new thinking. This isn't philosophy; it's the fascinating reality of how science evolves. Every scientific concept has its day: theories are born, experiments are designed, results are tested, and ideas are either disproven or accepted as canon 3 .
Compared to fifty years ago, citations now peak much more quickly, indicating that scientific ideas are evolving at an accelerated pace 3 .
The secret to measuring this intellectual heartbeat lies in an unexpected place: the humble citation. When scientists discuss an idea, they cite the paper that proposed it in their own work. Then, as the conversation moves on to fresh discoveries, references to the original paper gradually drop off. The rise and fall of these citations maps the lifespan of a paper's underlying ideas 3 .
Historically, this life cycle is changing dramatically. According to Jevin West, an information scientist at the University of Washington, this acceleration could stem from more scientists tackling problems, or from technology connecting them better and speeding up their conversations 3 . This invisible life cycle affects everything from which diseases get research funding to what technologies transform our daily lives.
Before an idea even reaches the stage of citations and peer review, scientists often use powerful imaginative tools to push thinking forward 6 .
These mental explorations allow scientists to ask "what if" in radical ways: "Imagine there is no oxygen in the atmosphere..." or "If we could travel through time..." 6 .
Different disciplines show distinct patterns in how quickly ideas spread and how long they remain influential 3 .
The most-cited papers have longer lifetimes than others. These often include methods papers that lay out experimental techniques others can use, or groundbreaking theories that continue to be cited for decades 3 .
In science, an experimentum crucis (Latin for "crucial experiment") is one capable of decisively determining whether a particular hypothesis or theory is superior to all other widespread explanations 4 .
The concept was first described by Francis Bacon in 1620 as instantia crucis ("crucial instance"), with the phrase experimentum crucis later coined by Robert Hooke and famously used by Isaac Newton and Robert Boyle 4 .
One of the most famous crucial experiments in scientific history occurred in 1919, when physicist Arthur Eddington led an expedition to Príncipe Island in Africa to observe a solar eclipse 4 . The goal was to test Albert Einstein's then-controversial general theory of relativity, published in 1915, which predicted that massive objects like the Sun would bend light from distant stars passing near them.
Einstein publishes his general theory of relativity
Eddington expedition to observe solar eclipse
Results presented at Royal Society meeting
At the time, Newtonian physics had dominated scientific thought for over two centuries. Einstein's theory made the startling prediction that light should be deflected by exactly 1.75 arc-seconds—double what Newton's laws predicted. The Eddington expedition represented a head-to-head showdown between the established Newtonian view and Einstein's radical new conception of the universe 4 .
Eddington's approach was methodical, designed to deliver unambiguous results:
Required a total solar eclipse to make stars observable near the Sun.
Multiple telescopes captured images of the star field around the eclipsed Sun.
Compared star positions during eclipse with their normal positions.
Expeditions to two locations to ensure findings weren't local anomalies.
This careful, repetitive methodology was crucial for producing results that would be accepted by the skeptical scientific community. The experiment took advantage of a natural celestial phenomenon to create laboratory conditions that couldn't be replicated on Earth.
When Eddington and his team developed their photographic plates and made precise measurements, the results were clear: the starlight had been deflected by an amount much closer to Einstein's prediction of 1.75 arc-seconds than the Newtonian value. The data from the experiment provided the first solid evidence in favor of Einstein's general theory of relativity 4 .
| Star Group | Measured Deflection (arc-seconds) | Newtonian Prediction (arc-seconds) | Einstein Prediction (arc-seconds) |
|---|---|---|---|
| Príncipe Results | 1.61 ± 0.30 | 0.87 | 1.75 |
| Sobral Results | 1.98 ± 0.12 | 0.87 | 1.75 |
The implications were revolutionary. As Eddington himself noted, the findings required scientists to fundamentally reconsider our most basic concepts of space, time, and gravity:
Einstein's theory proposed that gravity isn't a force in the traditional sense but rather the result of massive objects curving the fabric of spacetime itself.
The accurate prediction demonstrated the mathematical rigor of general relativity, suggesting it wasn't just a curious alternative but a more complete description of physical reality.
The results marked a dramatic departure from Newtonian physics that had stood unchallenged for centuries, showing that even our most established scientific "truths" could be refined or replaced.
"REVOLUTION IN SCIENCE - NEW THEORY OF THE UNIVERSE - NEWTONIAN IDEAS OVERTHROWN"
The experiment immediately catapulted Einstein to international fame and represented one of the most dramatic overturns of established science in history.
Contemporary analysis of citation patterns allows us to quantify how scientific ideas spread and evolve. The following data shows distinctive patterns across disciplines 3 :
| Scientific Field | Typical Citation Peak | Key Characteristics |
|---|---|---|
| Life Sciences | Flatter, longer citation trend | Ideas easier for experts across fields to grasp |
| Mathematics | Slower, later peak | Highly specialized language and concepts |
| Physical Chemistry | Multiple peaks for seminal papers | Some theories cited for decades |
| Environmental Science | Recent papers with many authors | Large collaborations becoming common |
Certain papers have exceptional longevity in scientific discourse. The most-cited papers generally fall into two categories, both with longer lifetimes than typical research 3 :
| Paper Type | Examples | Impact Duration |
|---|---|---|
| Methods Papers | Experimental techniques | Extended (often decades) |
| Foundational Theories | Quantum mechanics, Relativity | Very long (multiple decades) |
Behind every great experiment, including modern attempts to measure and understand scientific ideas themselves, lies a collection of essential research tools. These reagents and materials form the foundation of experimental science across disciplines:
| Research Reagent | Primary Function | Field of Use |
|---|---|---|
| Lithium aluminium hydride | Powerful reducing agent | Organic synthesis |
| Diisobutylaluminium hydride | Reduces esters and nitriles to aldehydes | Organic chemistry |
| Fenton's reagent | Oxidizes contaminants or waste waters | Environmental science |
| Sodium borohydride | Reduces ketones and aldehydes to alcohols | Biochemistry |
| Raney nickel | Desulfurization and hydrogenation catalyst | Organic synthesis & industrial |
| Silver nitrate | Abstract halides; precursor to other compounds | Inorganic chemistry |
| Fehling's reagent | Differentiates between aldehydes and ketones | Chemical analysis |
| Grignard reagents | Alkylation of aldehydes and ketones | Organic synthesis |
| Millon's reagent | Detects soluble proteins | Biochemical analysis |
| Collins reagent | Selectively oxidizes primary alcohols to aldehydes | Organic chemistry |
These reagents represent the fundamental tools that enable scientists to perform the reactions and analyses necessary to test their hypotheses and advance their fields 5 .
The 1919 Eddington expedition beautifully illustrates both the power of crucial experiments and the ongoing evolution of scientific ideas. While it provided compelling evidence for Einstein's theory, it didn't mark the end of gravity research. Instead, it opened new questions about black holes, dark matter, and the ultimate nature of the universe that physicists continue to explore today.
Where once scientific conversations played out over generations, today's digitally connected global research community can evaluate, adopt, or discard new theories in record time.
The life cycle of ideas continues to accelerate. This rapid cycling doesn't diminish the importance of foundational ideas like relativity, but rather reflects the growing pace of human discovery.
Perhaps the most profound insight from studying how scientific ideas evolve is recognizing that this process—with its crucial experiments, its citation patterns, its gradual acceptance and eventual superseding of theories—represents the most reliable method humanity has yet developed for understanding our universe. Each idea, whether it stands the test of time or is eventually overturned, represents an essential step in our collective journey toward greater knowledge.
This article was inspired by ongoing research into the nature of scientific discovery and the patterns of how knowledge evolves. For further exploration of these ideas, see the analysis by Popular Science on the life cycle of scientific ideas and the historical context of crucial experiments in science 3 4 .