The Nature of Science at Brookhaven Lab

On a secluded patch of land in central Long Island trees blocked any view of the buildings I knew were there. I paused my rental car at the guard station to receive a pass and drove cautiously as if something or someone was about to stop me. This is the campus of Brookhaven National Laboratory in Upton, New York, approximately 50 miles from Manhattan. Like many people I have an unsettled relationship with science. For me, it’s a what-could-have-been feeling mixed with you-made-your-choices. Decades ago, I wanted to be a scientist.

I’m exploring what access the public has to our national laboratory system. Magnificent in scale, these palaces of inquiry are more industrial than lush, but they elegantly balance mysteries with explanations. Unlike static Mt Rushmore, the Grand Canyon, or Statue of Liberty, our national labs are always a work in progress.

Before 1947 Brookhaven was a U.S. Army training camp. After the camp closed it grew into a national laboratory. Home to the first nuclear reactor in the United States. Home to the first reactor designed for medical research. And home to the soon to be Electron Ion Collider, which will explore how the proton got its spin and the still mysterious strong nuclear force that binds atomic nuclei together. The designated effort of the Department of Energy, Office of Science national labs is to solve human energy demands. That quest takes into account how the universe was formed, “seeing” matter’s building blocks, and learning from nature’s amazing ability to self-organize. I hope my enthusiasm will camouflage my Wikipedia-level knowledge of science.

The size of Brookhaven is deceptive. Its sprawling 5,280-acre campus is pocked with 300 buildings that catalog years of architectural history spanning from pre-industrial red brick low rise to LEED-certified modern steel frame.

The mammoth machines constructed here and the people who operate them hold the power to prove ideas right or wrong. They identify those with potential to change the future, or not. Either way, answers get found and new questions arise. So much begins here. This is the land of big science, basic science, experimental science, user science. The difference between ideas and experiments is as plain as that between a water faucet and white crested rapids. I grab my raft. I am thinking big, as in universe big, but the actual experience directs me to think small, as in atomic nuclei small.

I’m greeted by a manager in the Communications office and two staff members. I’m looking for a good reason to trust science, to come and see how science gets done, to be awed by science that benefits all humankind. We sat down at a large conference table where the manager click-started a Power Point presentation and handed me a site map. He’s been working at the lab for 27 years and still maintains excitement about his work. “No one really knows what it is like until they are here,” he said. I’m ready!

Our first stop is the Center for Functional Nanomaterials (CFN). At the CFN size matters. A nanometer is one billionth of a meter. A grain of salt or strand of hair is considered large in this microscopic world. I remember my first peek into a microscope was in a crowded fifth-grade Catholic school classroom with 55 students. When I asked my parents for a microscope, they thought it a ridiculous request for a girl.

Objects not only look different by scale, they behave differently. Think of the sounds coming from different sized pipes on a church organ. Or how light rays of different wavelengths emerge from a prism at different angles.

Scale helps scientists understand how nature self-organizes and opens the door to new energy efficient nanomaterials, as well as biological and industrial processes. Ash from forest fires and volcanic dust are naturally occurring nanomaterials.

Self-assembly is how evolution solves problems. In nature, if something is still here it knows how to exist. What are the structures that support that existence?

Through the eye of a moth

As an example, at the CFN observing the organic structure of a moth’s eye revealed an anti-reflective quality. This led Brookhaven scientists to create a nanotexture that increased solar cell efficiency. Like the eye of a moth, the solar cells harvest light rather than reflect it.

The glass walls, computers, and clean rooms in this building don’t suggest organic life to me. I can’t see what these scientists see. To me the shape of things are static. A leaf, a blade of grass can be held in my hand. I can draw a picture of it. However, depending on the scale, objects can be modified in different ways. At the macroscale, I can bend the blade of grass but the composition of it is static. At the nanoscale, I can’t bend the grass but its molecular structures can be modified.  For example, scientists can apply coatings containing organic molecules to develop a flexible shell. They learned to direct the organization of objects the way nature does, creating structures with new properties.

The idea is not new. Ancient Islamic potters and medieval European artists employed nanomaterials by grinding silver, gold and copper metals into powders to add luster to pottery and color to glass. Such uses were confirmed through electron microscopy and precision spectroscopy using laser light sources. In ancient India therapeutic processing of minerals and metals continues today in their Ayurvedic system of medicine. However, the scale to which scientists can “see” and direct nanoparticles is new.

A research team from Columbia Engineering and Harvard University used tools at Brookhaven’s CFN to view, measure, and image cross sections of butterfly wings at a nanoscale. Once thought to be useless membranes, the wings of butterflies were revealed to have incredible temperature control and a sophisticated sensory network. Such knowledge brought them closer to developing new radiative-cooling materials. Maybe one day advanced flying machines!

Before we leave CFN, I looked into a glass cubicle where two young scientists were crouched in chairs with their eyes fixed on computer screens. A pink hoodie encircled the woman’s neck. I could not hear their voices. They were like tigers scenting prey, unaware of our presence.

Let There Be Ultra Bright Light

The concrete floor in the building that houses the National Synchrotron Light Source II (NSLS-II) is clean to a shine. It is so expansive that scientists ride adult-sized tricycles to get from one area to another. Octopus like cables extend from the stainless-steel machines that sparkle under the fluorescent lights dangling high overhead. The quiet in this grand space is unexpected.

The National Synchrotron Light Source II building at Brookhaven.

Shining light on a metal knocks some of its free-flowing electrons out of the metal completely. The discovery of this law, called the photoelectric effect, landed Albert Einstein his one and only Nobel prize. At the NSLS II, electrons are extracted from materials such as metals then accelerated to circulate around the half-mile storage ring at a temperature hundreds of degrees below the freezing point of water. While racing around the ring, the electrons emit ultra-bright X-rays. However, emitting light causes the electrons to lose a bit of their stamina, so at a precise moment the electrons move through well-tuned superconducting cavities to gain their momentum back. Kind of like pushing a child on a swing. The NSLS-II shines its intense waves of light to “see” atoms that measure one-thousandth of a billionth of a meter. This kind of science led to advances in CT scan technology as well as discoveries in chemistry, matter physics, and biology.

Three of the beam lines here were used to characterize the atomic-level structure of viral components in COVID-19 and how they connect with receptors on human cells. Scientist from pharmaceutical companies, academia and Brookhaven lab collaborated in the search for antiviral agents and targets for vaccines.

From the sub, subzero cold environment inside the NSLS II we moved to the STAR (Solenoid Tracker) detector on the Relativistic Heavy Ion Collider (RHIC). A temperature that is 250,000 times hotter than the center of the sun is generated. Such contrasts intrigue me. I remember going from being popular to being ostracized the day my seventh-grade teacher announced I had received the highest grade on a science test.  Higher than the boy brainiacs? It was a fluke I told my fleeing friends who were more interested in go-go boots than how temperature impacts atoms.

STAR tracker

When we reached RHIC, the largest circular particle accelerator in the U.S., I’m introduced to a nuclear physicist who is flanked by coils, cables and pipes that make up STAR, a heavy ion detector stationed on RHIC’s 2.4-mile ring. STAR is as big as a house and I am invited in.

STAR detector

When I see the few women of my generation leading important science projects and the following generation of women achieving their goals in science, I realize that my career detour was only in part due to cultural and familial influences. What really halted my pursuit of science was high school math. I was terrible in math.

I saw only a fraction of what they do at Brookhaven and certainly didn’t understand all of it. It’s like being in the foothills with only a view of the mountains. Yet, any scientist will say there is always more to learn no matter where you start. This thought diminishes my regret of not being science savvy. I, like others who visit our national science labs, always want to know more.

In just a few hours my view of the world changed. I drove slowly on the road that led me away from the lab. Sunlight twinkled between the tree branches in a most perfect way. The autumn spray of color surrounded me. I smelled the musty ground that waited for leaves to fall. I imagined all the extras science will bring and all that nature has yet to reveal.

Star Power at Princeton

A poetic phrase on the U.S. Department of Energy’s website drew my attention to the Princeton Plasma Physics Lab (PPPL) in New Jersey. The phrase describes fusion energy sciences as “…bringing the energy-producing power of a star to Earth for the benefit of humankind.” Like most people, I’m not familiar with how fusion energy works and why it’s so difficult to obtain. But we’re all wondering if it can or will help save our planet from calamitous effects of climate change.

The PPPL plays a prominent role in plasma physics and fusion energy research. In 2019, through their website I registered to attend a public tour and encouraged my cousin Charlie to do so too. He agreed. He lives in Philadelphia, just 45 miles from Princeton. Now retired, Charlie formerly analyzed plastics for bio-chemical markets. He now likes working with wood. When I reach his house, he was pulling on a cable to charge his white Tesla sedan. Our journey to the lab would not emit any carbon into the beautiful blue sky overhead.

During the drive I tell him about the lab’s history. In 1951 during the Cold War a professor from Princeton received funding from the U.S. government to study and develop fusion power for weapons under a top-secret project called Matterhorn. A decade later the focus changed to basic research so the lab name changed too.

“I never would have thought of visiting a national lab,” Charlie says. Yet he is familiar with lab life. His father, my uncle Bob, was a chemical engineer at Oak Ridge National Lab in Tennessee. He worked on nuclear fission during another top-secret undertaking, the Manhattan Project. As we grow closer to Princeton Charlie admits to not knowing much about his father’s work. “He rarely talked about it. I guess I didn’t ask either.”

In Princeton we follow Scudder Mills Road to Campus Drive and curve around some tall trees before reaching the lab’s entry guard house. We show our registration papers and pass through. A security background check is made on all visitors prior to their attending the public tour.

Guard house at Princeton Plasma Physics Lab

Princeton Plasma Physics Lab entry guard house.

The goal of fusion research is to create sustainable energy much like the stars do. That means energy without greenhouse gases or long-term radioactive waste. The risk of accidents occurring with fusion is diminished because unlike fission which creates an uncontrolled chain reaction, a fusion reaction is controlled through a precise calculation of temperature, pressure and magnetic field. A disruption in any of these causes the reaction to end without incident.

Fusion’s promise as a clean, renewable source of energy has yet to fully pan out after 80 years of research. But that fact doesn’t dampen the enthusiasm of our guide, graduate student Oak Nelson.

“Oak? As in the tree?” Charlie asks after the young man introduces himself to our tour group. Bashfully, the tall lanky blonde-haired guide responds, “Yah. I grew up in Colorado.” He’s on break from classes and has time to be a guide before his next research project begins.

Plasma cloud

The lab’s lobby contains a lounge area where science-related posters hang on the walls. Against a windowed wall a hands-on plasma machine beckons visitors. I immediately gravitate towards the machine before the tour starts. I wait as two middle-aged women fiddle with its handle. By sliding and rotating the handle one can manipulate a magnetic field that pushes and swirls the plasma. The plasma appears as a pink, cloudlike smoke. The ladies allow me. I move the handle slowly at first and then quickly. The plasma cloud responds to my touch, billowing and thickening. I have no idea what it’s used for, but I feel powerful controlling it. The ladies tell me they live nearby and have long been curious about what happens inside this lab. “We are looking for something hopeful with all that’s going on in our country,” the tall one says. They nod to each other. I think they are referring to the political division in our country, but I say nothing in response.

Oak asks our group if anyone knows about plasma. No one raises a hand or speaks up. He explains it as a fourth state of matter where fusion reactions take place. “Ninety nine percent of the universe contains plasma,” he says. None of us knows about this? “Basically, plasma is very hot, charged gas,” he continues. Some of what plasma research has led to are computer chips and flat screen televisions.

We stop to eye what looks to me to be a modern work of sculpture. But it is actually a plasma containment device called a stellarator that was used in early nuclear fusion experiments. Relics such as this are to remind us of how far we’ve come.

Stellarator at Princeton Plasma Physics Lab

To explain fusion, Oak shows us a video with two animated nuclei portrayed as Pacman-like figures. They fuse together and ‘Pow!’ form heavier elements that release a lot of energy.

Fusion’s two sources of fuel are hydrogen and lithium, both plentiful on Earth. Oak is excited about something called ITER, pronounced “eater”. It’s a plasma physics experiment being conducted at CERN, the European organization for nuclear research in France. December of 2025 is the planned date for ITER to launch and create plasma that will reach temperatures of 150 million degrees Celsius. That’s about 10 times hotter than the center of our sun. Wow!

NSTX-U, apple versus doughnut

We move on to the National Spherical Torus Experiment Upgrade (NSTX-U). It’s the most powerful experimental fusion facility of its type in the world. Its design distinguishes it from others by using a cored apple shape rather than a larger doughnut shape. The hope is that the spherically shaped plasmas created could allow them to develop smaller, more economical and more stable fusion reactors. The big question here is can a machine be built where the energy produced surpasses the energy used to trigger and sustain the reaction. They are searching for the right recipe of heat and plasma density.

“We can change the planet with fusion,” Oak says as if the solution is at his fingertips. The challenge is on. Our sun’s core fuses 600 million metric tons of hydrogen per second.

The NSTX-U main control room looks similar to a lecture hall with banks of computers. It’s here where the power of high-speed computing, machine learning, simulators and models are pushing the perimeters that may lead to success. From there, we pass through an underground tunnel to enter a maze of thick copper-colored pipes that stand as walls and a ceiling at the base of NSTX-U.

Charlie and I climb a stair with the rest of the group. I ask a graduate student from Carnegie Mellon University why he came on the tour: “I’m studying computer science so am curious about how data is gathered and the simulations they use.”  A young Asian woman tells me she wanted to take the tour because her husband works here. At the top of the stair a young physician from Georgetown takes selfies with his father, who works as a mechanical engineer at the lab. His mom is a doctor. “My son takes after his mother,” the father jokes.

At different times we take turns stepping up to what I call the lookout platform. Instead of marveling at a deep canyon or distant forest, we peek at the top of the most powerful spherical tokamak (nuclear fusion reactor) in the world. There is no natural light, no windows or wind. No sound is emitted. A tennis-court-green grid surrounds the circular mouth of the tokamak. Inside is a stew of electrons and atomic nuclei. Red painted superconducting magnets and multi-colored cables bulge from its belly. A bank of electronic equipment records its every move. I don’t see any of the star part here – the shining light, the friendly twinkle or the streaking trail across a night canvas.

NSTX-U at Princeton Plasma Physics lab

Members of the public take turns viewing the NSTX-U at PPPL

Family members from Brazil approach the lookout platform snapping pictures. They are visiting a relative who works as a theoretical physicist here. The daughter in the family, Letica, says: “This is our future. My generation wants to know how we can live in a clean environment. It’s great to be a part of it.” The two middle-aged women I met in the lobby agree with her. “It’s terrific. Fascinating to see the work they are doing here.”

Before we leave the NSTX-U the Carnegie Mellon student asks: “How do you debug any problems?”

“Good question,” says Oak. “We had to call a retiree recently to diagnose a problem with the circuits. We’re glad he was available. This system has been growing organically for the last 20 years.”

Cousin Charlie smiles at the thought of a retiree coming in to fix it. “I guess it’s best to keep us around,” he says.

Public outreach

I had arranged in advance to meet with physicist Andrew Zwicker who heads the Office of Communications and Public Outreach at the lab. I asked him why they are optimistic now after decades of chasing the gold ring of fusion energy. He gives me a trio of reasons for why today’s optimism is not misplaced. “Our computing speed has increased tremendously. We use sophisticated simulators that allow us to tweak design easier. And advanced manufacturing capabilities allow us to create the components as needed.”

Zwicker tells me that their most popular public outreach program is the Ronald E. Hatcher Science on Saturday lectures. The lectures are held in the MGB Auditorium and have been ongoing for 34 years with an average of 300 people attending. They are live streamed at 9:30am EST for nine weeks from January to March. Any member of the public can watch live on the PPPL.gov website.

Princeton Plasma Physics Lab campus

End of the public tour at Princeton Plasma Physics Lab

Cousin Charlie sums up his thoughts on the tour as we walk to the parking lot: “I like the matter-of-fact personality of scientists. They want to find answers, not impose them like politicians do. That’s refreshing. It’s a precise, efficient operation here. The computers, modeling and prediction theory weren’t around when I was in school.”

I think of my master-of-the universe moment in the lobby when turning the handle to control the plasma machine. I ponder fusion science. Are we called to understand, emulate, one up the sun?

Charlie and I look for but don’t see any other electric cars in the lot. We spend the rest of the day in Princeton eating lunch at a farm-to-table restaurant, visiting the University Chapel and the Art Museum on Princeton’s main campus. During our drive back under the night sky I look up. My understanding of star power has forever changed. The crook in my neck assures me that my star wonder remains intact.

The search to harness fusion energy continues. In December of 2022 the U.S. Department of Energy announced an achievement of fusion ignition at Lawrence Livermore National lab. Scientists conducted the first controlled fusion experiment in history to produce more energy from fusion than the laser energy used to drive it. We will see where it goes from there.