Drexel Physics Seminar: Doctor Sowjanya Gollapinni on the current state of research on Neutrinos, the Ghost Particle of the Atom.

I took in a physics seminar at my old alma mater Drexel University on November 30th. I like to stop down once in a while to see what’s changed, a lot, as well as see who’s there that I still remember, seems like fewer each time.

The topic of the seminar was certainly one that interested me, Neutrinos; a kind of sub-atomic particle so difficult to detect it has been called a ghost particle. The German physicist Wolfgang Pauli first predicted the existence of neutrinos as a way of making the books balance in the radioactive process called beta (β) decay. Careful studies of the process showed that some energy was missing, and the angular momentum before and after didn’t match. Pauli suggested that if another particle was involved, one without electric charge and little or no rest mass, it could account for the differences while being very difficult to detect. The images below show the Nobel Laureate along with a diagram of the β decay process.

Wolfgang Pauli (Credit: Public Domain)
Beta Decay Process (Credit: Public Domain)

So difficult were neutrinos to detect that it took more than twenty years to prove that they existed. In fact neutrinos react with normal matter so rarely that while about ten billion (billion with a b) neutrinos are flying through your body every second only two or three will interact with a particle inside you during your entire life. Even today the way we study neutrinos is to arrange for zillions to fly through a detector so sensitive it can measure the properties of the one or two that interact.

Arranging that intense beam of neutrinos, and building that detector is the job of Doctor Sowjanya Gollapinni of the University of Tennessee at Knoxville. Dr. Gollapinni is one of the chief researchers of the MicroBooNE experiment currently running at Fermilab outside of Chicago along with being one of the chief designers of the future Deep Underground Neutrino Experiment (DUNE).

The MicroBooNE, BooNE stands for Boosting Neutrino Experiment by the way, is a new type of detector using a design known as a Liquid Argon Time Projection Chamber (LArTPC). In the detector scattering events (really just two particles bouncing off of each other) between neutrinos and Argon atoms occur inside a very large, uniform electric field. The electric field pulls the ionized atoms generated by the collision toward an incredibly fine mesh of detecting wires. The resulting data plots are then interpreted to determine the kind of neutrino (see below) as well as its energy. The images below show the first high-energy neutrino collision captured by MicroBooNE along with the first recorded cosmic neutrino event.

First Recorded Neutrino Event at MicroBooNE (Credit: MicroBooNE, Fermilab)
First Cosmic Neutrino event at MicroBooNE (Credit: MicroBooNE, Fermilab)

One of the reasons I like MicroBooNE so much is that it uses the Fermilab Tevatron as its source of high-energy neutrinos. The Tevatron was the world’s most powerful ‘atom smasher’ until the Large Hadron Collider (LHC) at CERN took the top spot in 2008. In the world of particle physics however being number two gets you nothing so the physicists at Fermilab have been working hard to reconfigure their equipment in order to continue to study new physics and MicroBooNE is a big part of that effort.

After talking about some of the results from MicroBooNE Dr. Gollapinni spent a little time talking about the next generation neutrino detector known as the Deep Underground Neutrino Experiment or DUNE. As shown in the figure below, DUNE will have two detectors, one just a short distance from the neutrino source at Fermilab while the second will be buried deep inside the Homestake Mine in South Dakota, a distance of 1300 kilometers away. When completed the DUNE detectors will be 400 times larger then MicroBooNE providing 400 time the data.

DUNE experimental setup (Credit: DUNE, Fermilab)

Now the reason for having a second detector a long distance away is to give the neutrinos produced at Fermilab time in order to change from one type or flavour of neutrino to another. You see one of the things we do know about neutrinos is that there are three flavours. One flavour is associated with the familiar electron, a second is associated with a particle called the muon who is like a heavy cousin of the electron while the third is associated with an even fatter cousin called the Tau particle. Even stranger is the fact that the three flavours will oscillate from one kind to another. Learning more about this oscillation process is one of the major goals of DUNE.

At the end of her discussion Dr. Gollapinni mentioned some preliminary but very exciting news. The results so far from MicroBooNE and several other neutrino experiments indicates, just indicates right now, the possible existence of a fourth flavour of neutrino, which would be a stunning result if proving to be true. Right now it’s just an indication, hopefully the DUNE experiment, scheduled to start collecting data in 2024, will give us the answer.

During the question period one of the students who were attending asked Dr. Gollapinni how many flavours of neutrino she thought there were and she answered ‘Well if we find a fourth it’ll be a Nobel Prize and that’s enough for me’.

I certainly wish her luck.

The Deep Underground Neutrino Experiment (DUNE) and why are Neutrinos so Important Anyway.

Over the past month or so I’ve published a series of posts describing what I see as the decline of science in America (28June to 12July2017). Well today I have some good news. Just this week construction has begun on the Deep Underground Neutrino Experiment or DUNE.

DUNE is a collaboration between two already existing physics labouratories. The Sanford Underground Research Facility (SURF) which is buried 2km deep in the old Homestake gold mine outside of Lead, South Dakota along with Fermilab outside of Chicago, the site of America’s most powerful particle accelerator, second only to the LHC at CERN in Europe.

By the way the Homestake mine first became a physics labouratory back in the 1960s when the first Neutrino telescope was build there to measure the flux of neutrinos coming from the Sun. An experiment that provided the first direct evidence that the Sun gets its energy from hydrogen fusion reactions.

The idea behind the DUNE experiment is that Fermilab will use its accelerator to generate an intense beam of the sub-atomic particles called Neutrinos, a particle that has been called the ghost particle because they only interact very rarely with other particles. To give you an idea of how rarely an interaction occurs, every second thousands of Neutrinos are going right through your body but over your entire lifespan only a handful will interact with a particle inside you.

That beam of Neutrinos from Fermilab will be aimed very precisely at SURF where the world’s largest Neutrino Detectors are now being installed. The 2000km trip underground will mean almost nothing to the Neutrinos; a few may be absorbed but only very a few. There will also be an identical detector array right at the output of Fermilab’s accelerator so that scientists can study what happens to the Neutrinos during their 2000km journey. The picture below shows a diagram of the planned setup of the DUNE experiment.

DUNE Experimental Layout (Credit: Fermilab)

You may ask, if only a few Neutrinos are absorbed in 2000km of rock won’t even fewer be captured by the detectors in South Dakota. Yes, absolutely, but the scientists will be able to measure precisely every characteristic of every single Neutrino that is detected.

So, what do the scientists hope to learn from DUNE, why are Neutrinos so important anyway? Well, first of all there is increasingly strong evidence that Neutrinos are actually far more numerous than the electrons and quarks that make up what we think of as matter. In a sense scientists simply don’t enjoy knowing so little about such an important particle.

There are some more well defined problems that we hope DUNE can help to solve. For one, the there’s the question why the Universe, or at least our part of it, is so dominated by matter with so little anti-matter. From all of our experiments at places like Fermilab the Universe should be composed of equal parts matter and anti-matter and Neutrinos may hold the key to understanding the imbalance.

Physicists also hope that a greater understanding of Neutrinos will give us greater insight into fundamental forces, gravity, electromagnetism and the nuclear forces. Understanding Neutrinos is also important because they play a large role in some of the most energetic events in the Universe, everything from supernova to black hole formation.

Despite the recent lack of support for science from our government it’s still true that America’s scientists are second to none and the DUNE project demonstrates how they will always find a way to do new and important work. If you’d like to read more about the DUNE experiment the links below will take you to the SURF and Fermilab WebPages for DUNE.

http://www.dunescience.org/

http://lbnf.fnal.gov/