The Seesaw Model

September 26, 2017
Neutrinos are very mysterious particles. They do not carry electric or magnetic charge, and so they do not interact very much with anything else. In fact we are constantly being showered with neutrinos from space that fly straight through us without interaction, and in fact straight through the entire Earth without even being slowed down. They are so difficult to detect that the weak nuclear decays that generate them were at first thought to be violating energy and momentum conservation since the scientists did not know they were producing neutrinos. And even when their existence was later predicted and proven, they continue to baffle physicists.

One of the main reasons is their mass. For decades they were thought to be massless, just like the photon is. However in the 1990s it was discovered that neutrinos produced in our Sun were oscillating between the three different neutrino species - and such time dependent oscillations are forbidden for a massless particle due to the effects of time dilation in the theory of relativity. So we knew then that neutrinos carried a mass, and yet countless other experiments had provided an upper limit on the mass that was several orders of magnitude smaller than the next lightest particles in the Standard Model. Twenty years later we still cannot explain why the neutrino should have a mass, and yet be so much lighter than everything else.

One option is a type of theory called a seesaw model

In the simplest of the seesaw models, there are three neutrinos that have similar properties to the Standard Model neutrinos, but are not exactly the same. Each of the three neutrinos is paired with a much heavier neutrino that has not yet been detected in experiments. Not only is this second neutrino heavier than anything we have yet detected, but in most of these models it is also assumed to not interact with anything else in the Universe. It is not affected by any of the three forces in the Standard Model (although it does still feel the effects of gravity). 

In this model, the light neutrino is massless and its partner can be as heavy as we need it to be. (The reason why the lighter one is massless instead of just very light is a technical issue of gauge symmetry, and is beyond the scope of this article).

The key aspect of the seesaw model is an interaction between these two neutrinos. We assume that there is some probability that a light neutrino can suddenly change into a heavy neutrino, and that similarly the heavy neutrino can change into a light neutrino. It is important to stress that this is not a decay of the heavy neutrino, and also that this is not the same type of oscillation that is observed in physical neutrinos, but rather an effect of quantum mechanics which a physical neutrino can be alternate between these two states.

In essence the physical neutrinos in the Standard Model are a combination of both the light and heavy neutrino states. We cannot observe either directly, but only their combination. It is then easy to calculate the masses of the two physically observable neutrino states, and we find that if the heavier state has mass M, then the lighter state will have a mass proportional to 1/M. This is where the models get their name from, as the two types of neutrino seesaw between themselves, and as an increase in the mass of one will decrease the mass of the other.

So the question then is what is intuitively happening here to provide the lighter neutrino with a mass? Essentially the physical neutrino behaves as a massless particle, with the same interactions and properties of the lighter neutrino state. Sometimes it will suddenly convert to a very heavy neutrino state and behave as a sterile, heavy neutrino. What we observe and measure in nature is an average of the two states' masses.

The heavier this heavy state is though, the less time the neutrino can spend in it. And so increasing its mass makes the physical neutrino heavier, but because it cannot stay in that state as long the overall effect is the lessen the apparent mass of the physical neutrino.

And so the final result is that the neutrino is a massless particle that sometimes will become very heavy, but only for a very brief moment. Then the physically observed neutrino is an average of the two, and appears to observers to be a very light, but not quite massless particle.

That is the Seesaw Model in a nutshell.

NB: In keeping with the theme of this blog, I have avoided giving the mathematical formulae for the seesaw models. However they are also quite interesting, and anyone who wishes to discuss them further is welcome to find me in the forums or e-mail me for more details.
 

The End of Cassini

September 15, 2017
After twenty years of studying the planet Saturn, the working life of the Cassini spacecraft will come to an end in the next few hours. On Friday, September 15, 2017 at about 7:55 am EDT, NASA will crash the probe into the surface of Saturn and end its mission.

As far back as the 1980s astronomers from around the world were making plans to send a probe to the gas giant, Saturn. We had already explored both Mars and Venus, and the Voyager probes had made flybys of the outer planets, but Saturn ...
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The HL-LHC

September 14, 2017
As students around the world return to school, or start college, or begin new coursework and training of other kinds, particle physicists are also starting new things in the form of new data runs from the Large Hadron Collider. The LHC has already produced evidence of the Higgs boson, and added further constraints to many other theories of nature. The next data run could easily find evidence of dark matter, dark energy, or even hidden higher dimensions in the Universe.

However the topic of tod...
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Back To School

September 5, 2017

Some loyal readers will recognize this entry as a repeat from the last three years. Each year it gets a good response, and kudos from my readers, and so as before I must appease my loyal followers...

To all the students starting University, enjoy this time of your life. Long ago when I started, a prof told me that this is the start of your real education. Now you get to choose your own courses and your own field of study. It is entirely up to you to decide what to do with this chance.

I know fr...


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Free Software

September 5, 2017
With the arrival of September, students around the world will be returning to classes this week. And for those who are starting out at college or university, one of the most important considerations is how to live on a budget. These are the years when one has little or no income, but must bear the expenses of living independently for the first time. While giving advice on living on a budget is far too expansive to cover in this blog, I can tackle one small aspect of student life by providing ...
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The Antihydrogen Spectrum

August 3, 2017
Another interesting result from the Canadian led team at the ALPHA collaboration, with a paper publish today in Nature in which they present the hyperfine spectrum of anti-hydrogen.

Anyone who has the least interest in either physics or astronomy is aware of atomic spectra. Over a century ago scientists discovered that each chemical element emits a signature series of wavelengths of light, which is unique to that element. From the colour of emitted light we can identify each element that is p...
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Ten Years of GalaxyZoo

July 11, 2017
Happy 10th Anniversary to the team behind the GalaxyZoo website!

Back in 2007 a group of astronomers set up this program that would provide images from professional telescopes to the public, and allow dedicated volunteers to classify the different types of galaxies that were visible. This has produced countless academic papers in peer reviewed journals, and has allowed an army of amateur scientists to have a real impact on our understanding of the Universe.

On a personal level, I was a graduate...
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Simpson's Paradox Visualized

July 10, 2017
A while ago I wrote an article about an interesting statistical phenomenon known as Simpson's Paradox. According to Simpson's Paradox, a company can have discriminatory hiring policies in spite of each of its individual departments being completely fair. A new medical treatment can work better than existing methods for both the young and the old, and yet it gives worse results when you don't know the age of the patient. And it can make a single data set produce opposite and contradictory resu...
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A Forty Year Old Mystery Is Solved

June 7, 2017
After forty years of speculations ranging from exotic particle decays to advanced alien civilizations, the famous 6EQUJ5 signal has now been explained, and the explanation is embarrassingly rather basic.

In August 1977, astronomers at the Big Ear observatory at Ohio State university were scanning the sky for radio signals from space. There are numerous sources of radio waves in the galaxy, and a lot of interesting science can be done using a map of the sources of radio signals. And of course m...
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X-Ray Navigation & Communication

June 1, 2017
Yesterday I wrote about the theory of neutron stars and pulsars, and about the NICER mission that is about to begin examining them in more detail. After fifty years of theoretical study and limited astronomical data, we are soon to have a dedicated x-ray telescope with the primary purpose of studying the composition and properties of pulsars in the galaxy.

However the mission has a second goal, and one with a more practical purpose than studying distant neutron stars and pulsars. The mission w...
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About Me


Dr. Chris Bird I am a theoretical physicist & mathematician, with training in electronics, programming, robotics, and a number of other related fields.

   


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