
"If I knew what I was doing, it wouldn't be research."
D.M. Winnicott
Presently I Am Concentrating On:
Testing Fundamental Symmetries with Trapped Antihydrogen
A primary reason for making measurements with antimatter is to try to find clues to one of the central mysteries of our time - namely, "Where is all the antimatter?" That is, in the Big Bang, matter and antimatter were created in equal amounts but the universe is now dominated by matter. This is a good thing as matter and antimatter annihilate each other so we wouldn't be around if this wasn't the case. But it still begs the question as to the mechanism that led to the disappearance of the primordial antimatter. You can hear me talk about this on the "Big Questions" Quirks & Quarks show broadcast June 21, 2014 as well as my "the star spot" podcast Where Have All the Antimatter Gone? broadcast on June 15, 2014. A few years ago I also gave a public lecture about this using as a central theme the movie "Angels & Demons" where antimatter is used as bomb (trailer alert: not possible, so relax). By the way, while there isn't a lot of it, it is still true that there is antimatter all around us - even coming from you ... and bananas! A nice discussion of antimatter is given in Ten things you might not know about antimatter (April, 2015) although, come on, admit it, you know at least 5 of them.
The ALPHA (Antihydrogen Laser PHysics Apparatus) experiment ( animation) is done at CERN's Antiproton Decelerator. The AD has been upgraded with a new deceleration ring ELENA which is to come online in 2021 (LS2 Report: waiting for antiprotons... - CERN News, October, 2020). ALPHA managed to produce and hold ("trap") antihydrogen atoms for as long as 1000s (2011), made the first measurment of microwave transitions in antihydrogen (2012), and measured the charge of antihydrogen (2014). The Canadian group on ALPHA was awarded the 2013 NSERC Polanyi Prize.
Not to toot our own horn or anything but in 2010 ALPHA along with another AD experiment called ASACUSA were named the Physics World Breakthrough of the Year. We were one of the finalists for the 2021 Breakthrough of the Year but ultimately Quantum entanglement of two macroscopic objects is the Physics World 2021 Breakthrough of the Year. You win some, you lose some.
Spectroscopic Measurements with ALPHA
Spectral lines can be measured with great precision. Comparing the spectral lines of antihydrogen with those of hydrogen allows for one of the most precise tests of the CPT Theorem (a kind of symmetry between matter and antimatter) which requires the lines to be exactly the same. CPT invariance is a fundamental requirement of a quantum field theory and the Standard Model, the theory that describes the interactions of elementary particles, is a quantum field theory. Finding deviations from CPT invariance would have enormous implications for physics and would require a rethink of our mathematical description of nature. A clear, detailed discussion of testing CPT (and gravity, see below) using trapped antihydrogen is given in the 2015 PhD thesis by Andrea Capra.
Here are some recent results:

- Precision spectroscopy of the hyperfine components of the 1S–2S transition in antihydrogen - nature physics, January 17, 2025
- Adiabatic expansion cooling of antihydrogen - Physical Review Research, September 16, 2024
- Laser cooling of antihydrogen atoms - nature, April 1, 2021
- The original paper by Fujiwara et al. that proposed doing this.
- A proposal for laser cooling antihydrogen atoms - Journal of Physics B 46, January, 2013 - Lasers could chill antihydrogen - physicsworld
- The original paper by Fujiwara et al. that proposed doing this.
- Investigation of the fine structure of antihydrogen - nature, February 19, 2020
- Observation of the 1S–2P Lyman-α transition in antihydrogen - nature, August 22, 2018
- Characterization of the 1S–2S transition in antihydrogen - nature, April 4, 2018
- Antihydrogen accumulation for fundamental symmetry tests - nature communications, September 25, 2017
- Observation of the hyperfine spectrum of antihydrogen - nature, August 3, 2017
- An improved limit on the charge of antihydrogen from stochastic acceleration - nature, January 20, 2016
Testing Gravity with ALPHA-g
Lately I've been concentrating on efforts to use trapped antihydrogen to test the gravitational interaction between matter and antimatter (so-called "antigravity"). Einstein's General Theory of Relativity was published (1916) seventeen years before the first observation of an antiparticle (the anti-electron or positron) and so, naturally, did not include any considerations of whether antiparticles would gravitate differently than particles. There have been many attempts over the years to implement antigravity although most (see for example, Schiff's 1958 paper) found it problematic. Nevertheless, as always, it is an experimental question! As said by Shel Silverstein in his poem "Falling Up"
I tripped on my shoelace
And I fell up -
Up to the roof tops,
Up over the town,
Up past the tree tops,
Up over the mountains,
Up where the colors
Blend into sounds.
But it got me so dizzy
When I looked all around,
I got sick to my stomach
And I threw down.
Anyway, towards this end, we designed and built a second optimized apparatus, called ALPHA-g. You can watch Timelapse videos of the construction in 2018 of the ALPHA-g apparatus in the ALPHA pit. It's really amazing how the pit got filled up with stuff!
Our first ALPHA-g paper - Observation of the effect of gravity on the motion of antimatter (nature, September 27, 2023) - detailed our finding for the free fall acceleration of antihydrogen of (0.75 ± 0.13 (statistical + systematic) ± 0.16 (simulation))g. This garnered a lot of attention around the world with headlines like;
- Scientists drop antimatter to see if it falls - CBC
- Scientists have observed antimatter free-falling due to gravity for the first time - CTV News
- Nothing’s the Matter With Antimatter, New Experiment Confirms - New York TImes
- Scientists get closer to solving mystery of antimatter - BBC
- Scientists find antimatter is subject to gravity - The Guardian
- Antimatter feels gravity's pull, and one of biggest mysteries of the Universe stays unsolved - Australian Broadcasting Corp
- Hence proved! Nothing's the matter with antimatter as it loses a bit more pizazz; reacts same under gravity - Hindustan TImes
- Mysterious antimatter observed falling down for first time - RFI (France)
- What Happens if You Drop Antimatter? New Gravitational Test Sees First Fall - Scientific American
- Antimatter falls like matter, upholding Einstein’s theory of gravity - Science News
- Antimatter definitely doesn't fall up, physicists confirm - New Scientist
- Antimatter embraces Earth, falling downward like normal matter: Study reveals gravity's effect on matter's elusive twin - PhysOrg News
- Antimatter does not fall up, CERN experiment reveals - physicsworld
- Antimatter Feels Gravity Just like Matter - APS physics
- Antimatter falls down, just like ordinary matter - Science
- Scientists Report Breakthrough Investigating Antimatter and Antigravity - Vice
- Antimatter Reacts to Gravity in the Same Way as Ordinary Matter, Physicists Find - Gizmondo
- With ‘Leaning Tower of Pisa-Type of Experiment’ Physicists Find Antimatter Affected by Gravity, Too - Sputnik International
- Does antimatter fall down or up? We now have a definitive answer - Popular Science
- »Super bedrift«: Efter 20 års eksperimenter beviser Aarhus-forsker, at antistof falder nedad - Videnskab DK (Denmark)
- Auch Antimaterie fällt nach unten - Suddeutsche Zeitung (Germany)
- "Einstein tenía razón": el descubrimiento que acerca a los científicos a resolver el misterio de la antimateria - la patilla (Spain)
While we found that antihydrogen is certainly not gravitationally repelled by the Earth, I believe it is technically incorrect to say that this is equvalent to the statement that antimatter is not gravitationally repelled by matter. The reason has to do with the mass constitution of the proton (and, therefore, due to CPT Conservation, of the antiproton). The 2018 Lattice QCD calculation of Yang et al. found that 32(4)(4)% of the mass of the proton is due to the kinetic energy of the quarks with the rest associated with gluon dynamics. The masses of the two up quarks and one down quark in the proton add only another 1% so the quark mass-energy contribution to the proton mass is ~33% and, therefore, due to CPT Conservation, only around one-third of the antiproton mass is actually due to antiquarks, i.e., is actually "antimatter". I explored the consequences of this fact in the following arXiv preprints;
- What Exactly is Antimatter (Gravitationally Speaking)? - arXiv:2401.10954 (January, 2024)
- Do We Live in an Antigravity Universe? - arXiv:2409.18145 (September, 2024)
- What Exactly is Antimatter (Gravitationally Speaking)? A Second Scenario - arXiv:2501.10589 (January, 2025)
One of the results presented in the third preprint is that it follows quite naturally from antigravity that the free fall acceleration of antihydrogen would be (0.78+0.11−0.08)g. The improbably good agreement with the ALPHA-g result shouldn't be taken terribly seriously but it is true that I found that the antihydrogen free fall acceleration would be positive (i.e., antihydrogen would fall down just like hydrogen) but more importantly it is constrained to be definitively less than g. It will be interesting to see if ALPHA-g can get the systematic errors down low enough to test this.
The part of ALPHA-g that I specifically worked on was antihydrogen detection using a tracking chamber (a so-called radial Time Projection Chamber or rTPC) and a scintillating cosmic ray veto detector. Here is some information about the rTPC:
- Design of a Radial TPC for Antihydrogen Gravity Measurement with ALPHA-g - September, 2016
- Design of a Radial TPC for Antihydrogen Gravity Measurement with ALPHA-g - June, 2016

Long-baseline Neutrino Experiments using Liquid Argon Time Projection Chambers (LArTPC)
- Neutrino oscillation physics using a large (15 to 50 kton) Liquid Argon Time Projection Chamber. The neutrino source could have been either the off-axis NuMI beam from Fermilab (subsequently using other technology), a future high intensity neutrino beam from Fermilab towards DUSEL (now realized as the DUNE experiment), or a future neutrino facility like a Neutrino Factory. Here is a nice video showing neutrino reconstruction for the NOvA experiment on which I was a collaborator for a while.
- I worked as a Fermilab Associate Scientist on the Neutrinos at the Main Injector (NuMI) project. The review of Fermilab carried out by the U.S. Department of Energy (where I presented the case for NuMI) is reported in the July 18, 1997 issue (note that it includes a rare picture of me on page 5 wearing a suit!) of Ferminews. The December 11, 2014 issue of Fermilab Today had a nice "Physics in a Nutshell" explanation of How to make a neutrino beam. Fermilab TM-2018, "Conceptual Design for the Technical Components of the Neutrino Beam for the Main Injector", is a fairly complete description of the NuMI neutrino program including a detailed description of the physics and technical elements of the neutrino beamline.
- Here is my contribution to educating the public about neutrinos. In this case, I was asked to respond to a question about neutrinos that was emailed to the Fermilab Public Affairs Office.
- It's been confirmed what we already suspected, Physicists Hail Major Breakthrough After Discovering Neutrinos Just Little Italian Neutrons! (July, 2020)
Muon Colliders
- One large advantage of lepton colliders such as the e+e- colliders LEP and SuperKEKB over hadron colliders like the proton-proton collider LHC is that all of the beam energy goes into the primary collision. That is, in a 91 GeV per beam collider like LEP, there is 182 GeV of energy available for new particle production since the collision is a point-particle on point-particle collision. At the LHC, on the other hand, the protons may have a kinetic energy of 7 TeV or so but the proton is not a point-particle and so that energy is shared among the constituents of the proton, the quarks and gluons. The actual point-particle collisions (the so-called "hard collision") are between constituents of the colliding protons and so the energy available for production of new particles is often considerably less than 14 TeV. Why not then just build a 14 TeV center-of-mass energy e+e- collider you ask? The answer is synchrotron radiation, the EM radiation emitted by charged particles when they are accelerated (as happens for a charged particle travelling in a circular path as in a collider). The problem is that for a given kinetic energy and accelerator radius, the power (energy/time) of the emitted radiation is inversely proportional to the 4th power of the mass of the particle being accelerated. Since the proton is around 2000 times as massive as the electron, then amount of synchrotron radiation emitted for an electron is 20004 times greater than for a proton. You can reduce this loss by increasing the radius but it puts a major limit on e+e- colliders and is the reason why LEP basically set the energy limit for circular colliders while the LHC uses the same tunnel but has beams with almost 100 times the energy.
- One could get around this to some extent (i.e., have the advantages of leptonic point-particle collisions but with much less synchrotron radiation loss) if there were a heavier lepton than the electron. Luckily there is - the muon. I have for many years (as in several decades) thought that muon colliders were the way to go. Oddly enough there are quite a number of other crazy souls out there as well as evidenced by this August, 2023 article from Scientific American - Particle Physicists Dream of a Muon Collider. There's also the November, 2021 article from APS News - Muon Colliders Hold a Key to Unraveling New Physics. Ah, to sleep, perchance to dream …
- Another the nice thing is that with a muon collider you also get a Neutrino Factory essentially for free. A Neutrino Factory was historically seen as a precursor to a Muon Collider since you don't need two (colliding) beams but just one. Here's a small sample of the various design reports, etc., over the years:
- Expression of Interest in R & D towards a Neutrino Factory Based on a Storage Ring and a Muon Collider - November, 1999
- From Neutrino Factory to Muon Collider - June, 2010
- The NuMAX Long Baseline Neutrino Factory Concept - May, 2018
- The future prospects of muon colliders and neutrino factories - March, 2019
Past Experimental Collaborations:
- The ZEUS experiment at the HERA accelerator located at the DESY laboratory in Hamburg, Germany, stopped taking data on June 30, 2007. For a history of DESY's change in emphasis from high-energy physics to "photon" physics have a look at Turning the Ship: The Transformation of DESY, 1993–2009. We were part of the team which constructed a new Strawtube Tracker (STT). The device was installed in early 2001 in order to greatly enhance the reach for high Q2 physics as well as heavy flavour physics.
- BTeV - the hadron collider CP Violation experiment at Fermilab. BTeV was summarily terminated by the U.S. Department of Energy on February 7, 2005 (in a press conference no less). See the Response from BTeV. It was all very sad.
- The CLEO experiment at CESR, the Cornell Electron Storage Ring.
- The BaBar Silicon Vertex Detector
- The Silcon Vertex Detector for the ALEPH experiment at the LEP collider at CERN.
- The Tagged Photon Spectrometer Collaboration (E691) at Fermilab.
- There is a rather funny article from the February, 1987, Chicago Tribune discussing what life was like for a young male at Fermilab at this time. (It has since improved .... a bit.)
- A (then young) theoretical physicist mentioned in the article, Marcello Gleiser, won the 2019 Templeton Prize
- There is a rather funny article from the February, 1987, Chicago Tribune discussing what life was like for a young male at Fermilab at this time. (It has since improved .... a bit.)
