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Discovering elusive particles with FASER

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Jamie Boyd, Co-Spokesperson for the FASER and FASERν experiments at CERN, discusses the aim of the projects and the potential impacts of recent discoveries on the field.

In March 2023, the Forward Search Experiment (FASER) published its first results, detecting collider neutrinos for the first time in an experiment environment.

FASER is one of the most recent particle physics experiments established at the Large Hadron Collider at CERN. The experiment started taking data in July 2022, and stopped taking data, for this year, in July 2023.

Designed to discover and study the elusive, weakly interacting particles that can be produced in collisions, the FASER experiment could help to solve some of the biggest mysteries in particle physics. By putting predictions to the test, the experiment refines our understanding of concepts such as dark matter, and enables us to confirm, exclude or possibly introduce predictions. Its subdetector, FASERν, studies interactions between high-energy neutrinos, developing our understanding of fundamental physics.

The Innovation Platform spoke with CERN Research Scientist and FASER Co-Spokesperson, Jamie Boyd, to learn more about the FASER and FASERν experiments, as well as the potential implications of recent discoveries on the field.

Can you explain the FASER and FASERν experiments and their objectives?

The FASER experiment was designed to search for hypothetical new particles that could be produced in the Large Hadron Collider (LHC) collisions. FASER is positioned in a special location, different to other experiments at the LHC, to be sensitive to new particles that could potentially be produced, but not seen, by other experiments.

The search is motivated by models that attempt to explain dark matter. Thanks to observations in space, we know about the existence of dark matter, and it can be explained by models that would potentially show new particles at the Large Hadron Collider.

The FASER experiment at CERN with Jamie Boyd

FASER is also designed to study high-energy neutrinos that are produced in LHC collisions. FASERν is a sub detector and is part of the FASER experiment designed to detect and study neutrinos.

Neutrinos are part of the standard model of particle physics, the theoretical framework that has been well-validated by experiments. However, they’ve never been studied when produced at a particle collider. At a collider, we can study the highest-energy neutrinos ever produced in a laboratory experiment. Though higher energy neutrinos have been studied coming from astrophysical sources, it has traditionally been difficult to know where they come from or what is producing them.

In the LHC collisions, we know the energy of the colliding protons, and consequently, we know how the neutrinos are produced, the energy they have, and can therefore study their interactions.

Typically, a new facility would be required to study such neutrinos, bringing associated large costs while also being time and labour-intensive. FASER allows us to take advantage of the neutrinos already being produced at the LHC. Utilising an existing facility in this way is very efficient, and we are truly maximising the physics that can be extracted from it.

What progress has been made since you began taking data in 2022?

We started taking data at the start of Run 3 of the LHC, in July 2022, and data was then taken continuously while the LHC was colliding protons, until November 2022. The process then began again in March 2023.

Using the data from 2022, FASER released two results for the Winter Conferences in March 2023. One of these was the search for a possible new particle that could help explain dark matter, the dark photon. An analysis was conducted to search for this dark photon, but unfortunately, it was not found. However, this did enable us to exclude certain dark photon lifetimes and masses, and consequently, refine the allowed parameters in the model.

An electron neutrino interaction candidate detected in the FASERν detector

Perhaps more exciting was the detection of neutrinos. Although we are familiar with these particles, we have yet to see collider neutrinos in an experiment environment, with these results marking their detection for the first time. Both the detector, and the experiment as a whole, operated very well. That neutrinos were highly visible in our data gives us conduct very interesting neutrino studies as more data is collected.

Why is it important that we understand neutrinos?

Neutrinos are a very elusive, fundamental particle in the standard model, interacting so weakly that they are hard to capture and study. Although, there’s a huge number of them, experimentally, they are difficult to measure. As a result, they have not been well understood.

The traditional method of studying neutrinos requires shooting a beam of particles into a fixed target that then intersects the beam and produces a shower of secondary particles. Among these secondary particles are neutrinos. However, such neutrinos are typically produced at between 100 and 1000 times lower energy than the ones observed in FASER.

There are several models beyond the standard model, designed to answer different types of questions in particle physics, and these can modify how neutrinos interact at high energy. With FASER, we will be able to constrain these models with data for the first time, using an unexplored energy.

Neutrinos from astrophysical sources are also important for studying and increasing our understanding of the universe.

Ice Cube is an experiment based in the Antarctic that uses the ice as a target to measure neutrinos coming from space. This enables us to look for dark matter, black holes, and effects yet to be discovered. These are very high-energy neutrinos, and understanding their interactions is an important element of utilising Ice Cube data to learn about fundamental physics.

The measurements of neutrinos made at FASER will help with this endeavour, and bring us closer understanding some of the most mysterious aspects of the universe.

In July, the teams at CERN quickly and expertly discovered and solved a leak in the LHC, did this affect the FASER experiment?

Although the leak was quickly fixed, the data produced since its repair has targeted experiments other than FASER. Therefore, FASER essentially finished taking data – for 2023 – earlier than expected, as a result of the leak.

However, we are operating at the very cutting edge of technology. The magnets of the LHC are the coldest place in the Universe, and operate under extreme vacuum. Problems such as these are therefore normal and anticipated.

What are the challenges faced when conducting a project like this?

The FASER location presents the biggest challenge, as it is very specific and difficult to access. The access route is narrow and, in some areas, it is highly radiated. It also requires walking along the LHC, which can’t be done while the accelerator operates.

These factors necessitate a robust detector rarely in need of maintenance. So far, this has been successful. The detector has worked as expected, and no intervention has been required during beam operation.

An experiment designed to operate in space is constructed under the assumption that it is inaccessible, meaning reliability is a necessity, and there must be contingencies in place that enable the project to operate, should parts break. The same principle is generally applied at CERN.

A display of a recorded muon event the FASER detector

To our advantage, at CERN there is an option to repair and access the experiments if necessary, which provides a degree of leeway. However, to do so interrupts the operation of the LHC and has ramifications across the entire CERN physics programme. Thus, to minimise intervention, the experiments are designed and built to be highly reliable and robust.

What does your recent neutrino discovery, with FASER, mean for the experiment?

FASER is a new experiment, constructed over the recent long shutdown and only in operation for little over a year. That the experiment operated as expected, and collider neutrinos were observed so quickly is really promising. The operations ran smoothly and the detector performance was excellent, a factor not guaranteed in an experiment of this kind.

As a young, small team, the effort required to achieve a project of this scale was significant, and therefore, the results are particularly rewarding. The results demonstrate the experiment’s successful design, which is encouraging news for the future of our operations, and enabling us to continue as anticipated.

Why is it such a significant development in the field?

Regarding the field in general, this particular result is a proof of concept. It proves we are capable of studying neutrinos at the LHC in the high-energy regime. As FASER takes more data in the next years, we will have the capacity and time to analyse our results more thoroughly, to extract useful – and possibly entirely novel – information about high-energy neutrinos.

The project marks an important new chapter in this area of physics, the results of which will be applicable to astrophysics and particle physics. These results are the first step towards utilising this experiment to better understand fundamental physics.

Please note, this article will also appear in the sixteenth edition of our quarterly publication.

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Here’s how Helene and other storms dumped a whopping 40 trillion gallons of rain on the South

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More than 40 trillion gallons of rain drenched the Southeast United States in the last week from Hurricane Helene and a run-of-the-mill rainstorm that sloshed in ahead of it — an unheard of amount of water that has stunned experts.

That’s enough to fill the Dallas Cowboys’ stadium 51,000 times, or Lake Tahoe just once. If it was concentrated just on the state of North Carolina that much water would be 3.5 feet deep (more than 1 meter). It’s enough to fill more than 60 million Olympic-size swimming pools.

“That’s an astronomical amount of precipitation,” said Ed Clark, head of the National Oceanic and Atmospheric Administration’s National Water Center in Tuscaloosa, Alabama. “I have not seen something in my 25 years of working at the weather service that is this geographically large of an extent and the sheer volume of water that fell from the sky.”

The flood damage from the rain is apocalyptic, meteorologists said. More than 100 people are dead, according to officials.

Private meteorologist Ryan Maue, a former NOAA chief scientist, calculated the amount of rain, using precipitation measurements made in 2.5-mile-by-2.5 mile grids as measured by satellites and ground observations. He came up with 40 trillion gallons through Sunday for the eastern United States, with 20 trillion gallons of that hitting just Georgia, Tennessee, the Carolinas and Florida from Hurricane Helene.

Clark did the calculations independently and said the 40 trillion gallon figure (151 trillion liters) is about right and, if anything, conservative. Maue said maybe 1 to 2 trillion more gallons of rain had fallen, much if it in Virginia, since his calculations.

Clark, who spends much of his work on issues of shrinking western water supplies, said to put the amount of rain in perspective, it’s more than twice the combined amount of water stored by two key Colorado River basin reservoirs: Lake Powell and Lake Mead.

Several meteorologists said this was a combination of two, maybe three storm systems. Before Helene struck, rain had fallen heavily for days because a low pressure system had “cut off” from the jet stream — which moves weather systems along west to east — and stalled over the Southeast. That funneled plenty of warm water from the Gulf of Mexico. And a storm that fell just short of named status parked along North Carolina’s Atlantic coast, dumping as much as 20 inches of rain, said North Carolina state climatologist Kathie Dello.

Then add Helene, one of the largest storms in the last couple decades and one that held plenty of rain because it was young and moved fast before it hit the Appalachians, said University of Albany hurricane expert Kristen Corbosiero.

“It was not just a perfect storm, but it was a combination of multiple storms that that led to the enormous amount of rain,” Maue said. “That collected at high elevation, we’re talking 3,000 to 6000 feet. And when you drop trillions of gallons on a mountain, that has to go down.”

The fact that these storms hit the mountains made everything worse, and not just because of runoff. The interaction between the mountains and the storm systems wrings more moisture out of the air, Clark, Maue and Corbosiero said.

North Carolina weather officials said their top measurement total was 31.33 inches in the tiny town of Busick. Mount Mitchell also got more than 2 feet of rainfall.

Before 2017’s Hurricane Harvey, “I said to our colleagues, you know, I never thought in my career that we would measure rainfall in feet,” Clark said. “And after Harvey, Florence, the more isolated events in eastern Kentucky, portions of South Dakota. We’re seeing events year in and year out where we are measuring rainfall in feet.”

Storms are getting wetter as the climate change s, said Corbosiero and Dello. A basic law of physics says the air holds nearly 4% more moisture for every degree Fahrenheit warmer (7% for every degree Celsius) and the world has warmed more than 2 degrees (1.2 degrees Celsius) since pre-industrial times.

Corbosiero said meteorologists are vigorously debating how much of Helene is due to worsening climate change and how much is random.

For Dello, the “fingerprints of climate change” were clear.

“We’ve seen tropical storm impacts in western North Carolina. But these storms are wetter and these storms are warmer. And there would have been a time when a tropical storm would have been heading toward North Carolina and would have caused some rain and some damage, but not apocalyptic destruction. ”

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Follow AP’s climate coverage at https://apnews.com/hub/climate

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Follow Seth Borenstein on Twitter at @borenbears

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Associated Press climate and environmental coverage receives support from several private foundations. See more about AP’s climate initiative here. The AP is solely responsible for all content.

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‘Big Sam’: Paleontologists unearth giant skull of Pachyrhinosaurus in Alberta

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It’s a dinosaur that roamed Alberta’s badlands more than 70 million years ago, sporting a big, bumpy, bony head the size of a baby elephant.

On Wednesday, paleontologists near Grande Prairie pulled its 272-kilogram skull from the ground.

They call it “Big Sam.”

The adult Pachyrhinosaurus is the second plant-eating dinosaur to be unearthed from a dense bonebed belonging to a herd that died together on the edge of a valley that now sits 450 kilometres northwest of Edmonton.

It didn’t die alone.

“We have hundreds of juvenile bones in the bonebed, so we know that there are many babies and some adults among all of the big adults,” Emily Bamforth, a paleontologist with the nearby Philip J. Currie Dinosaur Museum, said in an interview on the way to the dig site.

She described the horned Pachyrhinosaurus as “the smaller, older cousin of the triceratops.”

“This species of dinosaur is endemic to the Grand Prairie area, so it’s found here and nowhere else in the world. They are … kind of about the size of an Indian elephant and a rhino,” she added.

The head alone, she said, is about the size of a baby elephant.

The discovery was a long time coming.

The bonebed was first discovered by a high school teacher out for a walk about 50 years ago. It took the teacher a decade to get anyone from southern Alberta to come to take a look.

“At the time, sort of in the ’70s and ’80s, paleontology in northern Alberta was virtually unknown,” said Bamforth.

When paleontogists eventually got to the site, Bamforth said, they learned “it’s actually one of the densest dinosaur bonebeds in North America.”

“It contains about 100 to 300 bones per square metre,” she said.

Paleontologists have been at the site sporadically ever since, combing through bones belonging to turtles, dinosaurs and lizards. Sixteen years ago, they discovered a large skull of an approximately 30-year-old Pachyrhinosaurus, which is now at the museum.

About a year ago, they found the second adult: Big Sam.

Bamforth said both dinosaurs are believed to have been the elders in the herd.

“Their distinguishing feature is that, instead of having a horn on their nose like a triceratops, they had this big, bony bump called a boss. And they have big, bony bumps over their eyes as well,” she said.

“It makes them look a little strange. It’s the one dinosaur that if you find it, it’s the only possible thing it can be.”

The genders of the two adults are unknown.

Bamforth said the extraction was difficult because Big Sam was intertwined in a cluster of about 300 other bones.

The skull was found upside down, “as if the animal was lying on its back,” but was well preserved, she said.

She said the excavation process involved putting plaster on the skull and wooden planks around if for stability. From there, it was lifted out — very carefully — with a crane, and was to be shipped on a trolley to the museum for study.

“I have extracted skulls in the past. This is probably the biggest one I’ve ever done though,” said Bamforth.

“It’s pretty exciting.”

This report by The Canadian Press was first published Sept. 25, 2024.

The Canadian Press. All rights reserved.

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The ancient jar smashed by a 4-year-old is back on display at an Israeli museum after repair

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TEL AVIV, Israel (AP) — A rare Bronze-Era jar accidentally smashed by a 4-year-old visiting a museum was back on display Wednesday after restoration experts were able to carefully piece the artifact back together.

Last month, a family from northern Israel was visiting the museum when their youngest son tipped over the jar, which smashed into pieces.

Alex Geller, the boy’s father, said his son — the youngest of three — is exceptionally curious, and that the moment he heard the crash, “please let that not be my child” was the first thought that raced through his head.

The jar has been on display at the Hecht Museum in Haifa for 35 years. It was one of the only containers of its size and from that period still complete when it was discovered.

The Bronze Age jar is one of many artifacts exhibited out in the open, part of the Hecht Museum’s vision of letting visitors explore history without glass barriers, said Inbal Rivlin, the director of the museum, which is associated with Haifa University in northern Israel.

It was likely used to hold wine or oil, and dates back to between 2200 and 1500 B.C.

Rivlin and the museum decided to turn the moment, which captured international attention, into a teaching moment, inviting the Geller family back for a special visit and hands-on activity to illustrate the restoration process.

Rivlin added that the incident provided a welcome distraction from the ongoing war in Gaza. “Well, he’s just a kid. So I think that somehow it touches the heart of the people in Israel and around the world,“ said Rivlin.

Roee Shafir, a restoration expert at the museum, said the repairs would be fairly simple, as the pieces were from a single, complete jar. Archaeologists often face the more daunting task of sifting through piles of shards from multiple objects and trying to piece them together.

Experts used 3D technology, hi-resolution videos, and special glue to painstakingly reconstruct the large jar.

Less than two weeks after it broke, the jar went back on display at the museum. The gluing process left small hairline cracks, and a few pieces are missing, but the jar’s impressive size remains.

The only noticeable difference in the exhibit was a new sign reading “please don’t touch.”

The Canadian Press. All rights reserved.

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