What is a ‘neutrino’ and why
would we want to build a factory to produce them?
(Andrew Phillips)
What is the neutrino and where did it come from?
The
neutrino is a fundamental particle, as is the electron. This means that it has
not yet been broken down into any smaller constituents and therefore is
considered to be part of the universe’s family of basic building blocks. It was
originally believed to be mass-less and merely comprised of pure kinetic energy
but now physicists are of the opinion that it indeed has a mass but only of
small magnitude. It has no charge, a very low reaction cross-section (there is
a very low probability that it will react with any other matter) and only
really reacts via the ‘weak’ interaction which has an extremely short range.
This was the reason for the name given to it by Wolfgang Pauli in 1930 when he
proposed the existence of this elusive particle (neutrino: ‘little neutral
one’). In fact, even after predicting its existence, Pauli was doubtful that
scientists would ever successfully detect it by experiment. So the neutrino
actually ‘existed’ in the scientific world for around 26 years as a purely
theoretical particle whose purpose was to explain away the energy discrepancy
observed in beta decay experiments. It was only in 1956 that neutrinos were
experimentally detected for the first time and so physicists all around the
world working in the neutrino field could breathe again; their reputations
still intact!
But why?
There exist even greater motives to
power the search for neutrinos though, reaching beyond beta decay
experiments. More knowledge about the
nature of these neutrinos would provide valuable pieces to several rather
complex puzzles that have been perplexing physicists for many years now. Here
are a few of the major ones:
1)
The
Sun produces neutrinos in the fusion reactions which take place in its core.
Using their current knowledge of the workings of the Sun and neutrinos,
theoreticians predict a certain flux of neutrinos emitted from the Sun. So why
have experiments only successfully detected around half the neutrinos
previously expected? This problem is currently thought to be linked to neutrino
oscillations but is still under investigation.
2)
Astrophysicists
have observed an orbital angular velocity in stars rotating around galaxies
that is higher than predicted using gravity and mass calculations. This has
caused some scientists to challenge the theory of gravity. However, since it
has been decided that neutrinos have mass, they could be a part of the ‘dark
matter’, currently held responsible for this effect, and hold potential to
explain this extra orbital velocity.
3)
Cosmic
rays are very high-energy particles, which have been observed to have been
penetrating the Earth’s atmosphere. These particles interact with atmospheric
atoms to produce a ‘shower’ of new particles (some of which are neutrinos)
which can be detected on the Earth’s surface or in the atmosphere directly. A
great deal of mystery still surrounds this issue and there is belief that some
of these incoming cosmic rays could in fact be neutrinos.
4)
Another
point which is not so much of a puzzle but a key to a higher understanding of
the universe’s origins: it is believed that a large quantity of neutrinos were
generated during the Big Bang and once the cooling process began, many were
left to drift throughout the universe. This neutrino ‘sea’ has now cooled to
approximately 2K and learning more about these neutrinos would give insight
into the processes that took place in the early universe and led to the
existence of all the matter we see around us today.
So how can we detect neutrinos if they barely interact with other
matter?
Ironically,
even though neutrinos are some of the smallest particles to have ever been
studied, the detectors constructed to find them are some of the largest to have
ever been built. The problem lies in the low reaction cross-section (as
mentioned earlier), not lack of abundance. In fact there are billions of
neutrinos passing through your body every minute but they just slip by like
ghosts, unaffected. This giant melee of energies is of little use in terms of
scientific observation; with three neutrino ‘flavors’ in circulation we can
learn little about the properties of a neutrino. ‘Flavor’ is simply a term used
to define the interaction characteristics manifested by that particular
neutrino. For example, in most circumstances electron-neutrinos (ne) are involved in reactions with
electrons and muon-neutrinos (nm)
are involved in reactions with muons. The third neutrino is a tau-neutrino (nt) and is, unsurprisingly, involved
in reactions with the tau particle. This means that one needs collimated beams
with known flavors so that we can study time-dependent effects such as
oscillations (see later).
Machines
to generate and detect these beams have been proposed in several locations
worldwide. For example, Fermilab (US) have a project underway, in conjunction
with which the US Department of Energy has agreed to fund a mile long detector
to be built half a mile underground in the Soudan mines. There is also a
facility (NGS) under construction at CERN which will send a beam through the
Earth’s crust to a detector in Gran Sasso, Italy. No accelerating tunnels are
necessary due to the fact that the neutrinos are very unlikely to be involved
in any reactions on their journey.
The detector to be built in the
Soudan mines contains many plastic scintillation fibres and can only detect
neutrinos indirectly via the particles emitted in process known as reverse
beta-decay, should the neutrino happen to collide with an atomic nucleus. This
process generates a flash of light which signifies a neutrino event. With a
pure beam, such as the one proposed for CERN, it would be possible to observe
the neutrino flavor both at launch and detection points in order to confirm any
change in flavor, hence oscillation that might take place.
Neutrino oscillation was the
experimental evidence that confirmed the neutrino’s mass. It is due to a
phenomenon know as the ‘quantum- mixing’ of flavors, so that there is a
discrete probability that you will find any one neutrino with a certain flavor
at a certain time. Beams of neutrinos will therefore be in oscillation between
flavors on the journey from source to detector.
What happens now?
It would
seem as though the only scientific certainty that has confirmed its place in
the future of this research is the insatiable quest for knowledge which is
human curiosity. The mysterious and complex nature of neutrino physics, with so
many dependent theories resting in the balance, provides the perfect bait for
hungry minds.
One
especially mind-blowing consequence of this research was the discovery of
neutrino mass. This linked the particle nicely into a particularly cutting-edge
field of research: the Higgs particle. The Higgs particle has been proposed as
the mechanism by which all matter acquires mass, the stronger the Higgs field
interaction, the larger the mass. In its previous mass-less state, the neutrino
wouldn’t have been a candidate for investigation in this area of physics.
With
neutrino factories under construction, the hunt continues and so one can only
await further revelations from the search into our inner universe of the
unimaginably small.
References
·
NuMI-MINOS- Neutrino Physics
http://www-numi.fnal.gov/public/neutrinophysics.html
·
Minnesota Technology
http://www.itdean.umn.edu/itbp/technolog/mayjun99/neutrino.html
·
Neutrino History
http://wwwlapp.in2p3.fr/neutrinos/aneut.html
·
Neutrino Flavor
http://hep.bu.edu/~superk/osc.html