The Trinity Site From ‘Oppenheimer’ is a Reminder of the Horror of Nuclear Weapons

The test left behind only fragments of an otherwise vaporised tower that held the Trinity bomb. Viewing the tower’s remains at this remote, rigorously guarded site is a bewildering and sobering experience.

Christopher Nolan’s 2023 film Oppenheimer is a biopic about the theoretical physicist behind the atomic bomb. After watching the film, I was inspired to write about my visit to the actual Trinity site, where the first atomic bomb was detonated.

As part of my research on nuclear weapons and civil defence, I visited the Trinity site in 2015. Located in the desert in the southwest United States, the Trinity site is isolated, peculiar and disconcertingly mundane.

The tower that held the bomb is featured prominently in the Oppenheimer film. A small fragment of it exists today, as the rest of it was vaporised. It was deeply unnerving being near the remainder of the vaporised tower.

Arriving at the site

The Trinity site is open to the public for only a few hours twice a year, by permission of the U.S. Army. The predicted popularity of Oppenheimer’s release will possibly overcrowd the next open house on Oct. 21.

When I visited the site, I first had to make my way to a very remote area of the New Mexico desert. Arrival had to be well before sunrise to have any chance of being in the small group of persons granted entry.

Then, after waiting for hours at the secluded gate of an active missile and munitions testing range, I had to pass the rigour of a screening at an army checkpoint and closely adhere to a given set of rules and regulations verbatim. Our convoy, escorted by military police, then went to a more remote interior location of the missile testing range.

We stopped at a barren plain in the Jornada del Muerto – “dead man’s journey” – desert.

I then walked a half kilometre along a dirt path leading to the crater. A chain-link fence distinguishes the area surrounding the crater from the rest of the desert. The blast crater is flatter than it is concave. The fence is demarcated with black and yellow signs reading “Caution Radioactive Materials.”

Visiting the site

The main attraction at the Trinity site is a simple obelisk made of volcanic rocks marking Ground Zero. It was erected in 1965.

Adjacent to the obelisk, small fragments of the tower remained. In the distance, a low white structure shielded portions of the crater. Green glassy radioactive rocks, known as Trinitite litter the ground.

There are very few elements of interpretive information like what one would see at a museum. Military personnel dragged out a replica of the Fat Man bomb dropped on Nagasaki in 1945. It served to occupy the attention of most visitors, who perhaps anticipated more to see and do.

Vaporised tower

The most significant observation I made at the Trinity site was a small fragment of metal in the ground. It was a fragment of the tower, and proof of physicist Albert Einstein’s theory that mass is just a concentrated form of energy. And mass can turn to energy under the conditions of an atom bomb detonation.

Einstein’s famous equation E = mc² explains the energy released in an atomic bomb, but did not explain how to build one. Einstein and Oppenheimer were colleagues, and the task of developing the atomic bomb was designated to Oppenheimer and his crew.

The Trinity test demonstrated that humankind could tap the essence of the sun. The bomb worked, creating temperatures hotter than the sun’s 15 million degrees Celsius core. Hot gas radiated its energy in the form of x-rays, which heated the surrounding air, annihilating everything in their path. The phenomenon created a nuclear fireball.

The tower that held the bomb last existed at 5:28 a.m. on July 16, 1945. It was no longer in existence at 5:29 a.m., at the time the Trinity test commenced. The test vaporised the experimental structure, leaving behind a crater about 1.4 metres deep and 80 metres wide.

An obelisk marks the site of Ground Zero. Photo: Samat Jain/Flickr, CC BY-SA 2.0.

Entertainment from horror

Oppenheimer is the latest film that explores the history of the atomic bomb. Other films go beyond this summer’s blockbuster to depict the full horror of what Oppenheimer created.

Jon Else’s 1981 documentary, The Day After Trinity, shows the real history behind Nolan’s Oppenheimer. The 1983 made-for-TV movie, The Day After, dared to show the uncomfortable images of nuclear Armageddon to American audiences. And Mick Jackson’s 1984 British television show Threads is one of the scariest depictions of nuclear war.

Watching the fake tower at the set of the Trinity site being vaporised in the Oppenheimer film’s version of the first atom bomb explosion is stunning. Especially in 70-millimetre IMAX screenings of the film.

Seeing the fragments of the real vaporised tower in the midst of a radioactive crater strewn with green glass rocks at the real Trinity site was a bewildering and sobering experience.

Jack L. Rozdilsky, Associate Professor of Disaster and Emergency Management, York University, Canada.

This article is republished from The Conversation under a Creative Commons license. Read the original article.

‘Questionable’: A Quiz by The Wire, July 22, 2023 Edition

Take this third edition of our quiz!

Questionable by The Wire is a mosaic of the fortnight’s developments, featuring coverage from the mainstream press as well as off the beaten path, and ensuring a special focus on fighting misinformation.

Take this third edition of our fortnightly quiz and see if you’re as caught up with the news as you think you are!

In this week’s edition, we are trying out a new format with the help of Google Sheets. Let us know what you think by writing to us at .

 

Review: Enrico Fermi, the Quiet ‘Pope’ in a Collapsing World

The Pope of Physics, by Bettina Hoerlin and Gino Segrè, is an informative biography of Fermi that also manages to deepen the sense of quiet mystery surrounding the legendary physicist.

The Pope of Physics, by Bettina Hoerlin and Gino Segrè, is an informative biography of Fermi that also manages to deepen the sense of quiet mystery surrounding the legendary physicist

Enrico Fermi. Credit: Enrico Fermi Collection, Atomic Heritage Foundation

Enrico Fermi. Credit: Enrico Fermi Collection, Atomic Heritage Foundation

Most books that are good are also useful as a result, and vice versa. Sadly, The Pope of Physics – a biography of the Italian-American physicist Enrico Fermi that is written in a style as flat and dry as the Mojave – is an exception. Its goodness is difficult to find but its usefulness is immediately apparent. No other biography of Fermi is as authoritative as this one, although with regard only to his early years. The book is filled with anecdotes from that period that help understand his famously clinical nature.

Fermi made lasting contributions to quantum mechanics, nuclear physics, cosmology and chemistry. It is impossible to walk a few paces down these roads without stumbling upon a marker saying, “Fermi was here”. Growing up in Italy, he was a bright student of physics learning under an old guard dismissive of the new-fangled quantum theories. He was also a philosopher of science racing against his contemporaries in Germany, the Netherlands and England to extend the ideas of Max Planck to explain nature’s fundamental constituents. A key figure in his early years was Orso Corbino, a physicist and statesman who ensured Fermi received all the important university admissions and appointments, who kept things moving for Fermi despite the political upheavals then rocking Italy.

The authors, Bettina Hoerlin and her husband Gino Segrè, nephew of Fermi’s student Emilio Segrè, are to be thanked for deftly fleshing out a young Fermi through the pages of history. Born in 1901, he lost his brother at a young age, was an apprentice in a farm for some time, married a Jewish girl, drove a car reputed for breaking down and became known as the future of Italian physics. As a physicist, he was famous for his ability to make quick sense of problems and simplify calculations to their essence in a jiffy. His students playfully claimed Fermi had “an inside track to god”. At the Via Panisperna, where the physics department of La Sapienza – the University of Rome – was located, he was nicknamed Il Papa, The Pope. Corbino was Padreterno, the Almighty himself.

The regime marches closer

It was also at the Via Panisperna in 1934 that Fermi and his colleagues discovered the potential of neutrons – slowed down to a particular speed – to cause nuclear activation, a precursor to the atomic bomb as well as the nuclear power plant. The first time their experiment was conducted, the setup led Fermi into confusing fission products for transuranic elements. This was a stroke of luck because it prevented the technology from falling into the hands of the fascist Benito Mussolini and his Nazi ally across the border. But as the political climate worsened, Fermi, his family and most of his colleagues were forced to emigrate from Italy. Mussolini would enact the Leggi razziali in 1938, legalising racial discrimination against the country’s Jews (of whom the physicist’s wife Laura was one).

Unsure of how he would make his ‘escape’, Fermi was helped by Niels Bohr, who told him that he was going to win the Nobel Prize for physics that year. So on December 6, 1938, Fermi flew to Stockholm with his family to collect the prize, from there flew to New York on January 2 and used the prize money to settle down. And it is after this point that The Pope of Physics loses its sheen. Fermi’s life in the US has been much better documented than his life before and that is what keeps the book interesting for as long as it does. In fact, the most significant of his contributions in the US are synonymous with the dawn of the Atomic Age, and books about the dawn of the Atomic Age have been abundant given the moment’s political consequences.

Gino Segrè and Bettina HoerlinThe Pope of Physics: Enrico Fermi and the Birth of the Atomic AgeHenry Holt, 2016

Gino Segrè and Bettina Hoerlin
The Pope of Physics: Enrico Fermi and the Birth of the Atomic Age
Henry Holt, 2016

At the same time, it is interesting to consider Fermi’s political affiliations. The man was known for being closed off and that further contributed to his reputation of being a clinical and forthright theorist. The Pope of Physics quotes Nella, his daughter, as saying, “It wasn’t that he lacked emotions, but that he lacked the ability to express them.” But then, there are those moments that make one wonder if there ever was any turmoil behind that pokerfaced visage.

For example: Hoerlin and Segrè write about how Fermi, though aware of Mussolini’s actions while being shielded from them by Corbino, accepted an opportunity to join the Royal Academy (set up to rival the Accademia dei Lincei) while in Italy – at the request of Mussolini – and had his salary doubled, joined the Fascist Party and turned down an apprentice because of the latter’s manifest antifascist sentiments. In the mid 1930s, he laboured with the motif “physics as soma”, ‘soma’ being a stress-relieving substance that plays a major role in the society of Aldous Huxley’s Brave New World (1932), as a way to sidestep the theatre of Italian politics.

He only noticed how dark the clouds over the horizon had become when Hans Bethe, Felix Bloch, Rudolf Peierls, Georges Placzek and Edward Teller had stopped visiting Via Panisperna because they were “searching for safe havens in the United States and the United Kingdom”, when Italy’s invasion of Ethiopia and participation in the Spanish Civil War made the atmosphere at home more polarised and, finally, when the Boys – what the physicists at Via Panisperna were called – themselves began to emigrate to escape Mussolini’s and Hitler’s Jewish persecution laws.

A clash of commitments

In another example, in 1939, when Fermi was to make a presentation before US Navy officials about the threat of a German nuclear weapon, The Pope of Physics reads (emphasis added):

Rather than dramatically conveying the German threat, as [Leo] Szilard or [Eugene] Wigner would doubtlessly have done, Fermi was his low-key self. Without embellishment, he laid the facts before the navy officials. In retrospect, the group may have made a mistake in choosing Fermi since he tended to downplay dangers. Those present at the briefing apparently concluded that there was no cause for alarm. The meeting was treated as a courtesy call; no further action would be required.

Neither did Fermi see the need to act further. He was interested in the challenge of producing a chain reaction and not eager to deal with the extra complications of political or military involvement. Fermi only wished to proceed with experimenting. He was also happy to see that the experiments he and [Herbert] Anderson were planning to conduct were similar to the slow neutron ones he and the Boys had performed a few years earlier in Via Panisperna.

Three years later, though he would oppose the American construction of the more-powerful hydrogen bomb down the line, calling it tantamount to “an act of genocide”, Fermi was not just closely involved with the Manhattan Project but was also part of a committee that, in June 1945, called for the bomb to be dropped without warning on an inhabited city.

In both instances, spanning a period from the 1920s to the 1940s, Fermi was supposed to have remained apolitical whereas his colleagues – ranging from the self-assured James Franck to the visibly agitated Szilard – were often thinking of the best ways to stall Hitler’s march to obtaining a nuke as well as to prevent the loss of hundreds of thousands of lives. Fermi thought that scientists weren’t equipped to make the best military decisions, but how easily can this choice be consigned to disinterestedness after having called for ‘The Gadget’ to be used in a surprise attack on a city? Was it a conveniently blinkered worldview?

Indeed, where was the clash of commitments to science and duties on the one hand and to moral sense and conscience on the other, exemplified by J. Robert Oppenheimer’s agony as the first bomb was tested and Karl Darrow’s anxious doubts about the bomb’s meaning as the ash floated down upon Nagasaki, inherent to this part of history? “At some level, he was able to treat the bomb blast as just another physics experiment”, the book reads. In another instance, a single line writes off any discomfiture that may have arisen after Fermi witnessed the Trinity test: “… while he was seemingly infallible, he was also human.” In a third, it quotes Szilard: “The struggles of our time did not affect Fermi very much, and he is no fighter”, as if to excuse Il Papa from judgment.

A harsh vantage point

While it is disturbing to realise a celebrated scientist made it big on the back of fascism, on the back of ignoring one’s political responsibilities except until it affected one personally, Hoerlin and Segrè seem so caught up with fawning over Fermi’s accomplishments that they often climb into the ivory tower after him. This is what makes The Pope of Physics seem like a fond remembrance more than an honest chronicle, leave alone a rigorous investigation, of a man who birthed the Atomic Age. They speak of his gaiety and placidity in moments of incredible tension, of his being an excellent swimmer in the icy waters of Lake Michigan while others would fall behind, of his solving problems until the moment he passed away – all trivia after having skirted the tougher details.

But as fond remembrance, The Pope of Physics is worthy of praise for picking the eyes of Enrico Fermi – perhaps the most reticent of all notable scientists – to see the biggest moments of the 20th century through. It is braver still to have the book reviewed in late 2016 and early 2017, when nationalism is sweeping across the world, economic protectionism is on the rise and people are once again emigrating to escape war on humans (as well as the climate). Given the nature of the times in which this book was written, Fermi’s views – and the indifference of its authors – seem even more inexplicable.

Remembering C.V. Vishveshwara, the Quasimodo of Black Holes

Vishveshwara inspired several generations of Indian physicists. Many of the internationally acclaimed among them testify to having been profoundly influenced by him at some point in their career.

Vishveshwara inspired several generations of Indian physicists. Many of the internationally acclaimed among them testify to having been profoundly influenced by him at some point in their career.

C.V. Vishveshwara. Credit: International Centre for Theoretical Sciences, Bengaluru

C.V. Vishveshwara (1938-2017)
Credit: International Centre for Theoretical Sciences, Bengaluru

Professor C.V. Vishveshwara, who passed away in Bengaluru recently, was one of the true pioneers of black hole physics. Vishveshwara belonged to a class of physicists who were attracted to Albert Einstein’s theory of general relativity under the influence of the legendary American physicist John Wheeler in the 1960s.

Born in 1938 to scholar C.K. Venkata Ramayya and K. Venkatasubbamma, Vishveshwara spent his schooldays in Bengaluru and later went to Mysore University to study physics. In the 1960s, he was a graduate student at the University of Maryland working with Charles Misner, a prominent relativist and former student of Wheeler. After spending a few years at the NASA Institute of Space Studies, New York University, Boston University and the University of Pittsburgh, he returned to Bengaluru in 1976 to take up a professorship at the Raman Research Institute. He later moved to the Indian Institute of Astrophysics, in the same city, where he formally retired from his professorship in 1998. However, he never stopped working.

Work on quasi-normal modes

One of the most important contributions of Vishveshwara was the mathematical proof of the stability of Schwarzschild black holes. In 1916, the German physicist-astronomer Karl Schwarzschild discovered a mathematical solution to Einstein’s equations that describe how spacetime curves around a non-rotating spherical object. If such an object is smaller than a characteristic radius, called its Schwarzschild radius, it would be enveloped by a strange surface called the event horizon. This event horizon would allow things to pass inwards – into the spherical object – but would prevent everything, including light, from coming out.

Wheeler would later coin the term ‘black hole’ to describe these objects. One important question in the 1960s was whether the Schwarzschild solution is mathematically stable under perturbations. This means that, for such an object to exist in the physical world, it should retain its form even when perturbed by something, like infalling matter or radiation. Otherwise, the object would break apart “if an ant sneezed in its vicinity”.

A black hole being perturbed by a sneezing ant. Cartoon by C.V. Vishveshwara. (Proc. of the 'Einstein Centenary Symposium’ held at Ahmedabad in 1979, Ed. A R Prasanna et al. Wiley Eastern, 1980)

A black hole being perturbed by a sneezing ant. Cartoon by C.V. Vishveshwara. (Proc. of the ‘Einstein Centenary Symposium’ held at Ahmedabad in 1979, Ed. A R Prasanna et al. Wiley Eastern, 1980)

Building upon earlier work by Tullio Regge and Wheeler, Vishveshwara showed in 1970 that the Schwarzschild black hole is indeed stable under perturbations. Earlier, theoretical calculations by J. Robert Oppenheimer and Hartland Snyder had showed that black holes could be produced in the gravitational collapse of massive stars. Vishveshwara’s analysis suggested that, if black holes are indeed produced, they would also continue to exist. Soon after, astrophysical evidence of the existence of black holes started coming in from X-ray observations. And today, black holes have become commonplace phenomena in astronomy.

Vishveshwara’s most celebrated work is the discovery of the so-called quasi-normal modes of black holes. Black holes are the simplest macroscopic objects in the universe. And the simplest of black holes – the Schwarzschild black hole – is completely described by a single parameter: its mass. In other words, the only thing to know about a Schwarzschild black hole is its mass; everything else about the black hole can be derived from its mass. This property is popularly expressed by the saying “black holes have no hair”.

In 1970, Vishveshwara showed that if we perturb a Schwarzschild black hole by throwing a pulse of gravitational radiation at it, the black hole would go back to its original state by emitting gravitational waves of a simple, characteristic form, called quasi-normal modes. The signal is analogous to the ringing down of a bell, which has a pure tone (i.e. single frequency) and a decaying amplitude. Frequencies of the quasi-normal modes are independent of the nature of the perturbation and are fully characterised by the mass of the black hole. Irrespective of whether we perturb a black hole by throwing a pulse of gravitational radiation, electromagnetic radiation or broken television sets at it, the emitted quasi-normal modes will have the same frequencies.

“The assertion that the black hole has no hair is probably the ultimate application of Ockham's razor,” says C.V. Vishveshwara. Another of his cartoons depicts Ockham shaving the hair off a black hole using his razor. (Proc. of the 'Einstein Centenary Symposium’ held at Ahmedabad in 1979, Ed. A R Prasanna et al. Wiley Eastern, 1980)

“The assertion that the black hole has no hair is probably the ultimate application of Ockham’s razor,” says C.V. Vishveshwara. Another of his cartoons depicts Ockham shaving the hair off a black hole using his razor. (Proc. of the ‘Einstein Centenary Symposium’ held at Ahmedabad in 1979, Ed. A R Prasanna et al. Wiley Eastern, 1980)

Later, this result was generalised to the case of rotating (or Kerr) black holes as well (named for Roy Kerr). Here, the quasi-normal modes are functions of two parameters of the black hole: its mass and its spin angular momentum. The observation of quasi-normal modes is considered to be a smoking-gun evidence of a black hole. Recently, the first observation of gravitational waves by LIGO gave us the first potential observational glimpse of quasi-normal modes. The final part of the observed signal, produced by the coalescence of two black holes, is fully consistent with what we expect from the quasi-normal mode ringing of a perturbed black hole produced by the merger. Future gravitational wave observations will strengthen this claim. Quasi-normal modes provide us a unique probe to the true nature of black holes.

A great inspiration

Vishu, as Vishveshwara was popularly known, inspired several generations of Indian physicists, especially relativists. Many internationally acclaimed Indian physicists testify to have been profoundly influenced by Vishu at some point in their career. The founding director and lifelong patron of the Jawaharlal Nehru Planetarium in Bengaluru, Vishu was deeply committed to the spread of scientific temper and knowledge among members of the civil society.

At the planetarium, he initiated a rigorous training program in physics for students from the city’s colleges. Several young students, who were trained through the Research Education Advancement Programme in Physical Sciences (REAP) that he initiated, are now prominent scientists in the country. A cartoonist par excellence, Vishu also had a remarkable sense of humour and a kind heart. He liked to call himself the “Quasimodo of black holes”, after the hunchback who rings the bell of the cathedral of Notre-Dame in Victor Hugo’s famous novel.

While his friends, colleagues and students mourn the loss of Vishu, they also celebrate his life and work.

Parameswaran Ajith is a physicist at the International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bengaluru.

Good Year for Science on Stage as Kidman Discovers the Double Helix in Photograph 51

A new play about Rosalind Franklin – the scientist whose crystallography work helped James Watson and Francis Crick discover DNA, but who never received the recognition she deserved – has taken London by storm.

A new play about Rosalind Franklin – the scientist whose crystallography work helped James Watson and Francis Crick discover DNA, but who never received the recognition she deserved – has taken London by storm

Nicole Kidman YouTube 51Photograph 51 is causing a stir in London (running through November at the Noel Coward Theatre) – and not just because the star of the show is Nicole Kidman. It’s also because of the gripping scientific story Anna Ziegler’s new play tells.
Kidman plays Rosalind Franklin, the scientist whose crystallography work helped James Watson and Francis Crick discover DNA, but who never received the recognition she deserved. In particular, her 51st photograph confirmed their hypothesis that the structure of DNA had to be a double helix. Until then they lacked this crucial evidence for their theory.

The production has been hailed by critics: in the New York Times Ben Brantley calls Kidman “pretty close to perfection” while Michael Billington in the Guardian wishes this “intriguing, informative 95-minute play” were longer. In many ways, it is an all-too-familiar tale: a woman working in a field dominated by men whose work was not given proper credit – a tragic figure who died too young (Franklin died of ovarian cancer at age 38).

Science on stage

Photograph 51 is one of several new “science plays” to have appeared this year (although it was first produced off Broadway five years ago, to positive reviews but to relatively little attention). In January, Tom Stoppard’s The Hard Problem played at the National Theatre, sold out for its entire run. This latest drama of ideas from the author of Arcadia (1993) is set in a well-funded institute for brain research and explores such questions as whether there is a neural basis for consciousness and whether humans are hard-wired for altruism.

The Hard Problem overlapped with Tom Morton-Smith’s Oppenheimer. That play explored J Robert Oppenheimer’s rise to prominence as leader of the Manhattan Project and his complex network of relationships with fellow physicists, the US military and his family and friends. Among other things, it probed the motives and ethics of using atomic bombs at Hiroshima and Nagasaki, questions that continue to haunt us 70 years on.

And yet another new science play, Informed Consent by Deborah Zoe Laufer, has just finished a successful run in New York. Based on real events, it explores the complex ethical issues arising from a genetic anthropologist’s research on the gene pool in an isolated Native American tribe in the Grand Canyon. Like Photograph 51, The Hard Problem and Shelagh Stephenson’s 1998 play An Experiment with an Air-Pump, Informed Consent features a female scientist and centres on the science and wider implications of genetics.

photograph-51-2

Popular science

So Photograph 51 closes out a bumper year for science in the theatre, especially plays by women and about female scientists. It also raises the question of what makes a successful science play. One of the central issues, raised most prominently by Michael Frayn’s 1998 play Copenhagen, is fidelity to historical events and people, such as Franklin, Oppenheimer, Bohr and Heisenberg.

What was Rosalind Franklin really like? Kidman’s portrayal of her exudes iron will and self-control. Her fellow scientists find her, as Brantley puts it: “exacting, humourless, brilliant and disciplined to the point of rigidity” – an intimidating and relentless perfectionist. But the Franklin family have claimed that although they’re pleased about the play’s public righting of the wrong done to her, the play misrepresents her personality. They also say it exaggerates the extent to which Franklin was a bold feminist pioneer. Scientific accuracy is also a contentious issue and is the subject of much debate between scientists and theatre makers.

What is common to science plays is the relentless search for knowledge – and this is key to their attraction for audiences. One of the central themes of Copenhagen and of Stoppard’s Arcadia is the importance of “wanting to know”, something that also comes across forcefully in Photograph 51. Kidman’s face as she studies the revelatory photograph exudes the thrill of discovery, of those eureka moments of science that make all the hard work, tedious repetition, and failure worth it.

Interestingly, that photograph is never shown to the audience, although it is reprinted in the programme. What the audience does see on stage is a post-war landscape strewn with rubble: a stark visual reminder of the circumstances in which these groundbreaking scientific advances are taking place.

Why now?

Although “science plays” have a long history, there is a particularly strong interest in putting science on stage right now. This is perhaps because there is a greater sense of urgency about what science can do, both for good and evil. As Oppenheimer (and its predecessor, a 1964 documentary play by Heinar Kipphardt about Oppenheimer) reminds us, World War II and the Cold War made it clear in an unprecedented way that science can have dire repercussions. Therefore, we all have an obligation to understand that and we all have a stake in it, not just the scientists and their funders.

And the way that we have access to seemingly endless information on medical issues, scientific findings and their implications on the internet has also helped science to burst the bounds of the laboratory.

Equally, the rise of “public engagement” initiatives has not just encouraged, but mandated scientists to speak to the public about their work. Many contemporary “science plays” are the result of new funding initiatives to enable public engagement, for instance by the Wellcome Trust and the Alfred P. Sloan Foundation in America, which helped to fund Informed Consent, for example.

As new areas of science open up, so too will new “science plays” emerge. Currently, climate change is enjoying an outing on the stage, with a spate of new productions dealing with global warming and its consequences. Who knows what will be next.The Conversation

Kirsten Shepherd-Barr, Professor of English and Theatre Studies, University of Oxford

This article was originally published on The Conversation. Read the original article.