ALPHA experiment

Last updated
Antiproton decelerator
(AD)
ELENA Extra low energy antiproton ring – further decelerates antiprotons coming from AD
AD experiments
ATHENA AD-1 Antihydrogen production and precision experiments
ATRAP AD-2 Cold antihydrogen for precise laser spectroscopy
ASACUSA AD-3 Atomic spectroscopy and collisions with antiprotons
ACE AD-4 Antiproton cell experiment
ALPHA AD-5 Antihydrogen laser physics apparatus
AEgIS AD-6 Antihydrogen experiment gravity interferometry spectroscopy
GBAR AD-7 Gravitational behaviour of anti-hydrogen at rest
BASE AD-8 Baryon antibaryon symmetry experiment
PUMA AD-9 Antiproton unstable matter annihilation
ALPHA experiment CERN Antimatter factory - Alpha experiment.jpg
ALPHA experiment

The Antihydrogen Laser Physics Apparatus (ALPHA), also known as AD-5, is an experiment at CERN's Antiproton Decelerator, designed to trap antihydrogen in a magnetic trap in order to study its atomic spectra. The ultimate goal of the experiment is to test CPT symmetry through comparing the respective spectra of hydrogen and antihydrogen. [1] Scientists taking part in ALPHA include former members of the ATHENA experiment (AD-1), the first to produce cold antihydrogen in 2002.

Contents

On 27 September 2023, ALPHA collaborators published findings suggesting that antimatter interacts with gravity in a way similar to regular matter, supporting a prediction of the weak equivalence principle. [2] [3]

Experimental setup

Working with antimatter presents several experimental challenges. Magnetic traps—wherein neutral atoms are trapped using their magnetic moments—are required to keep antimatter from annihilating with matter, but are notoriously weak. Only atoms with kinetic energies equivalent to less than one kelvin may be trapped. The ATHENA and ATRAP (AD-2) projects produced antihydrogen by merging cold plasmas of positrons and antiprotons. While this method has been quite successful, it creates antimatter atoms with kinetic energies too large to be trapped. Moreover, to do laser spectroscopy on these antimatter atoms, they need to be in their ground state, something that does not appear to be the case for the majority of antimatter atoms created with this technique.

Antiprotons are received from the antiproton decelerator and are 'mixed' with positrons from a specially-designed positron accumulator in a versatile Penning trap. The central region where the mixing and thus antihydrogen formation takes place is surrounded by a superconducting octupole magnet and two axially separated short solenoid "mirror-coils" to form a "minimum-B" magnetic trap. Once trapped, antihydrogen can be subjected to study, and the measurements compared to those of hydrogen.

Antihydrogen detection

In order to detect trapped antihydrogen, ALPHA also includes a 'silicon vertex detector': a cylindrical detector composed of three layers of silicon strips. Each strip acts as a detector for the charged particles passing through. By recording how the strips are excited, ALPHA can reconstruct the traces of particles traveling through the detector. When an antiproton annihilates, the process typically results in the emission of 3 or 4 charged pions. By reconstructing their traces through the detector, the location of the annihilation can be determined. These traces are quite distinct from those of cosmic rays also detected, but due to their high energy they pass straight through the detector.

To confirm successful trapping, the ALPHA magnet that creates the minimum B-field was designed to allow rapid and repeated de-energizing. The decay of current during de-energization has a characteristic duration of 9 ms, orders of magnitude faster than similar systems. In theory, the fast turn-off speed and the ability to suppress false cosmic rays signals allows ALPHA to detect the release of single antihydrogen atoms during de-energization.

Cooling antihydrogen

One of the main challenges of working with antihydrogen is cooling it enough to be able to trap it. Antiprotons and positrons are not easily cooled to cryogenic temperatures, so in order to do this ALPHA has implemented a well known technique from atomic physics known as evaporative cooling. [4] State-of-the art minimum-B traps such as the one ALPHA uses have depths of order 1 Kelvin.

Results

A preliminary experiment conducted in 2013 found that the gravitational mass of antihydrogen atoms was between −65 and 110 times their inertial mass, leaving considerable room for refinement using larger numbers of colder antihydrogen atoms. [5]

ALPHA has succeeded in the laser cooling antihydrogen atoms, a technique known as that was first demonstrated on normal matter in 1978. [6] [7] [8]

On 27 September 2023, the ALPHA team published a paper supporting the prediction that the gravitational interaction of antimatter is similar to that of regular matter. For the weak equivalence principle of general relativity to be correct, it is required that the two substances display identical gravitational properties. [2] [3] The findings rule out a 'repulsive [antigravity]', as previously theorized by some in the field.

Collaborators

ALPHA collaborators include the following institutions:

Related Research Articles

<span class="mw-page-title-main">Antimatter</span> Material composed of antiparticles of the corresponding particles of ordinary matter

In modern physics, antimatter is defined as matter composed of the antiparticles of the corresponding particles in "ordinary" matter, and can be thought of as matter with reversed charge, parity, and time, known as CPT reversal. Antimatter occurs in natural processes like cosmic ray collisions and some types of radioactive decay, but only a tiny fraction of these have successfully been bound together in experiments to form antiatoms. Minuscule numbers of antiparticles can be generated at particle accelerators; however, total artificial production has been only a few nanograms. No macroscopic amount of antimatter has ever been assembled due to the extreme cost and difficulty of production and handling. Nonetheless, antimatter is an essential component of widely available applications related to beta decay, such as positron emission tomography, radiation therapy, and industrial imaging.

<span class="mw-page-title-main">Positron</span> Anti-particle to the electron

The positron or antielectron is the particle with an electric charge of +1e, a spin of 1/2, and the same mass as an electron. It is the antiparticle of the electron. When a positron collides with an electron, annihilation occurs. If this collision occurs at low energies, it results in the production of two or more photons.

<span class="mw-page-title-main">Antimatter rocket</span> Rockets using antimatter as their power source

An antimatter rocket is a proposed class of rockets that use antimatter as their power source. There are several designs that attempt to accomplish this goal. The advantage to this class of rocket is that a large fraction of the rest mass of a matter/antimatter mixture may be converted to energy, allowing antimatter rockets to have a far higher energy density and specific impulse than any other proposed class of rocket.

<span class="mw-page-title-main">Antihydrogen</span> Exotic particle made of an antiproton and positron

Antihydrogen is the antimatter counterpart of hydrogen. Whereas the common hydrogen atom is composed of an electron and proton, the antihydrogen atom is made up of a positron and antiproton. Scientists hope that studying antihydrogen may shed light on the question of why there is more matter than antimatter in the observable universe, known as the baryon asymmetry problem. Antihydrogen is produced artificially in particle accelerators.

<span class="mw-page-title-main">Antiproton</span> Subatomic particle

The antiproton,
p
, is the antiparticle of the proton. Antiprotons are stable, but they are typically short-lived, since any collision with a proton will cause both particles to be annihilated in a burst of energy.

ATHENA, also known as the AD-1 experiment, was an antimatter research project at the Antiproton Decelerator at CERN, Geneva. In August 2002, it was the first experiment to produce 50,000 low-energy antihydrogen atoms, as reported in Nature. In 2005, ATHENA was disbanded and many of the former members of the research team worked on the subsequent ALPHA experiment and AEgIS experiment.

The Antihydrogen Trap (ATRAP) collaboration at the Antiproton Decelerator facility at CERN, Geneva, is responsible for the AD-2 experiment. It is a continuation of the TRAP collaboration, which started taking data for the TRAP experiment in 1985. The TRAP experiment pioneered cold antiprotons, cold positrons, and first made the ingredients of cold antihydrogen to interact. Later ATRAP members pioneered accurate hydrogen spectroscopy and observed the first hot antihydrogen atoms.

<span class="mw-page-title-main">PAMELA detector</span>

PAMELA was a cosmic ray research module attached to an Earth orbiting satellite. PAMELA was launched on 15 June 2006 and was the first satellite-based experiment dedicated to the detection of cosmic rays, with a particular focus on their antimatter component, in the form of positrons and antiprotons. Other objectives included long-term monitoring of the solar modulation of cosmic rays, measurements of energetic particles from the Sun, high-energy particles in Earth's magnetosphere and Jovian electrons. It was also hoped that it may detect evidence of dark matter annihilation. PAMELA operations were terminated in 2016, as were the operations of the host-satellite Resurs-DK1. The experiment was a recognized CERN experiment (RE2B).

<span class="mw-page-title-main">Gravitational interaction of antimatter</span> Theory of gravity on antimatter

The gravitational interaction of antimatter with matter or antimatter has been observed by physicists. As was the consensus among physicists previously, it was experimentally confirmed that gravity attracts both matter and antimatter at the same rate within experimental error.

<span class="mw-page-title-main">PS210 experiment</span> Scientific experiment

The PS210 experiment was the first experiment that led to the observation of antihydrogen atoms produced at the Low Energy Antiproton Ring (LEAR) at CERN in 1995. The antihydrogen atoms were produced in flight and moved at nearly the speed of light. They made unique electrical signals in detectors that destroyed them almost immediately after they formed by matter–antimatter annihilation.

<span class="mw-page-title-main">Antiproton Decelerator</span> Particle storage ring at CERN, Switzerland

The Antiproton Decelerator (AD) is a storage ring at the CERN laboratory near Geneva. It was built from the Antiproton Collector (AC) to be a successor to the Low Energy Antiproton Ring (LEAR) and started operation in the year 2000. Antiprotons are created by impinging a proton beam from the Proton Synchrotron on a metal target. The AD decelerates the resultant antiprotons to an energy of 5.3 MeV, which are then ejected to one of several connected experiments.

Atomic Spectroscopy and Collisions Using Slow Antiprotons (ASACUSA), AD-3, is an experiment at the Antiproton Decelerator (AD) at CERN. The experiment was proposed in 1997, started collecting data in 2002 by using the antiprotons beams from the AD, and will continue in future under the AD and ELENA decelerator facility.

High-precision experiments could reveal small previously unseen differences between the behavior of matter and antimatter. This prospect is appealing to physicists because it may show that nature is not Lorentz symmetric.

AEgIS, AD-6, is an experiment at the Antiproton Decelerator facility at CERN. Its primary goal is to measure directly the effect of Earth's gravitational field on antihydrogen atoms with significant precision. Indirect bounds that assume the validity of, for example, the universality of free fall, the Weak Equivalence Principle or CPT symmetry also in the case of antimatter constrain an anomalous gravitational behavior to a level where only precision measurements can provide answers. Vice versa, antimatter experiments with sufficient precision are essential to validate these fundamental assumptions. AEgIS was originally proposed in 2007. Construction of the main apparatus was completed in 2012. Since 2014, two laser systems with tunable wavelengths and synchronized to the nanosecond for specific atomic excitation have been successfully commissioned.

<span class="mw-page-title-main">GBAR experiment</span> Experiment at the Antiproton Decelerator

GBAR, AD-7 experiment, is a multinational collaboration at the Antiproton Decelerator of CERN.

<span class="mw-page-title-main">Buffer-gas trap</span> Device used to accumulate positrons

The buffer-gas trap (BGT) is a device used to accumulate positrons efficiently while minimizing positron loss due to annihilation, which occurs when an electron and positron collide and the energy is converted to gamma rays. The BGT is used for a variety of research applications, particularly those that benefit from specially tailored positron gases, plasmas and/or pulsed beams. Examples include use of the BGT to create antihydrogen and the positronium molecule.

The rotating wall technique is a method used to compress a single-component plasma confined in an electromagnetic trap. It is one of many scientific and technological applications that rely on storing charged particles in vacuum. This technique has found extensive use in improving the quality of these traps and in tailoring of both positron and antiproton plasmas for a variety of end uses.

<span class="mw-page-title-main">John H. Malmberg</span> American physicist

John Holmes Malmberg was an American plasma physicist and a professor at the University of California, San Diego. He was known for making the first experimental measurements of Landau damping of plasma waves in 1964, as well as for his research on non-neutral plasmas and the development of the Penning–Malmberg trap.

<span class="mw-page-title-main">Penning–Malmberg trap</span> Electromagnetic device used to confine particles of a single sign of charge

The Penning–Malmberg trap, named after Frans Penning and John Malmberg, is an electromagnetic device used to confine large numbers of charged particles of a single sign of charge. Much interest in Penning–Malmberg (PM) traps arises from the fact that if the density of particles is large and the temperature is low, the gas will become a single-component plasma. While confinement of electrically neutral plasmas is generally difficult, single-species plasmas can be confined for long times in PM traps. They are the method of choice to study a variety of plasma phenomena. They are also widely used to confine antiparticles such as positrons and antiprotons for use in studies of the properties of antimatter and interactions of antiparticles with matter.

<span class="mw-page-title-main">Jeffrey Hangst</span> Experimental particle physicist

Jeffrey Scott Hangst is an experimental particle physicist at Aarhus University, Denmark, and founder and spokesperson of the ALPHA collaboration at the Antiproton Decelerator (AD) at CERN, Geneva. He was also one of the founding members and the Physics Coordinator of the ATHENA collaboration at the AD facility.

References

  1. Madsen, N. (2010). "Cold antihydrogen: a new frontier in fundamental physics". Philosophical Transactions of the Royal Society A . 368 (1924): 3671–82. Bibcode:2010RSPTA.368.3671M. doi: 10.1098/rsta.2010.0026 . PMID   20603376. S2CID   12748830. Archived from the original on 2020-03-29. Retrieved 2021-07-22.
  2. 1 2 Overbye, Dennis (27 September 2023). "Nothing's the Matter With Antimatter, New Experiment Confirms - Consider it good news, physicists say: "The opposite result would have had big implications."". The New York Times . Archived from the original on 27 September 2023. Retrieved 28 September 2023.
  3. 1 2 Anderson, E. K. (27 September 2023). "Observation of the effect of gravity on the motion of antimatter". Nature . 621 (7980): 716–722. doi: 10.1038/s41586-023-06527-1 . hdl: 20.500.11850/636368 . PMC   10533407 . PMID   37758891.
  4. Grossman, Lisa (2010). "The Coolest Antiprotons". Physics. 26. American Physical Society. Archived from the original on 4 July 2010. Retrieved 2010-07-02.
  5. The ALPHA Collaboration & A. E. Charman (2013). "Description and first application of a new technique to measure the gravitational mass of antihydrogen". Nature Communications. 4: 1785. Bibcode:2013NatCo...4.1785A. doi:10.1038/ncomms2787. PMC   3644108 . PMID   23653197. Article number: 1785.
  6. Baker, C. J.; Bertsche, W.; Capra, A.; Carruth, C.; Cesar, C. L.; Charlton, M.; Christensen, A.; Collister, R.; Mathad, A. Cridland; Eriksson, S.; Evans, A. (2021). "Laser cooling of antihydrogen atoms". Nature. 592 (7852): 35–42. Bibcode:2021Natur.592...35B. doi: 10.1038/s41586-021-03289-6 . ISSN   1476-4687. PMC   8012212 . PMID   33790445.
  7. Wineland, D. J.; Drullinger, R. E.; Walls, F. L. (1978). "Radiation-Pressure Cooling of Bound Resonant Absorbers". Physical Review Letters. 40 (25): 1639–1642. Bibcode:1978PhRvL..40.1639W. doi: 10.1103/PhysRevLett.40.1639 . ISSN   0031-9007.
  8. Neuhauser, W.; Hohenstatt, M.; Toschek, P.; Dehmelt, H. (1978). "Optical-Sideband Cooling of Visible Atom Cloud Confined in Parabolic Well". Physical Review Letters. 41 (4): 233–236. Bibcode:1978PhRvL..41..233N. doi:10.1103/PhysRevLett.41.233. ISSN   0031-9007. Archived from the original on 2023-09-29. Retrieved 2021-07-22.

Record for ALPHA experiment on INSPIRE-HEP