Friday, October 24, 2014

Tullio Regge passed away

Tullio Regge (July 11, 1931 in Turin - October 23, 2014 in Orbassano)

Theoretical physicist and mathematician Tullio Regge, aged 83, passed away yesterday. He gave fundamental contributions to scattering theory (the theory of Regge poles is named after him) and to General Relativity among many other fields. His "Regge calculus" -based on a discretization of spacetime- is still widely used in Loop Quantum Gravity.

The relevance of Regge's heritage in modern physics is well shown by the fact that something like half of my papers cite the so-called Regge-Wheeler equation which describes how a Schwarzschild black hole vibrates after a perturbation and how it emits gravitational waves. The Regge-Wheeler equation was found in the late 1950s, even before the very concept of "black hole" (a name coined by Wheeler only in the 1960s) was formulated.

The Italian Institute for Nuclear Physics has dedicated its homepage to this news, more details on Regge's work can be found here.

Friday, October 17, 2014

The brightest pulsar ever

Last week the astrophysics community was hit by an exciting news. A very luminous X-ray source located in the "Cigar" galaxy M82 was discovered to be a spinning neutron star (a pulsar) rather than a black hole, as all models have assumed so far. This research was lead by astrophysicist Matteo Bachetti, who also happens to be a writer of this blog. Thus, we take the opportunity to ask Matteo a couple of questions whose answers you will not find in the excellent press (and radio) coverage that has followed the publication of this discovery.




Q: Matteo, first of all congratulations for what sounds like a great scientific achievement! How would you explain this discovery to my grandma? 


Thursday, September 18, 2014

Running Citizenship

Today's historical referendum in Scotland gives me the opportunity to talk about something I have in mind since I came back from the U.S. earlier this year. It's actually a very trivial concept that originates from the fact that:

When outside Europe, I feel European. When within Europe, I feel Southern European/ Mediterranean. When in Southern Europe, I feel Italian and, finally, when in Italy I definitely feel Sardinian. 

There is actually no contradiction in this Matrioska-like sense of belonging and I'm sure most people who happen to live abroad (which is already a rather subjective concept....) share the same feeling.

Anyway, this is interesting because in physics there is a much deeper and far-reaching concept that is (vaguely) related to the one above: that of the running couplings. In a quantum field theory, the coupling "constants" that define the strength of the couplings among quantum fields are not really constant, but actually their values depend on the energy scales.

As an example, take the most famous coupling constant, Newton's gravitational constant G that appears in the gravitational force law

F= G*mass1*mass2 / distance^2

which simply means that the intensity of the gravitational force between two masses (mass1 and mass2) is proportional to the masses and inversely proportional to the square of the distance. The proportionality factor is nothing but what we use to call Newton's constant and its value is G~6.673×10^{-11} N·(m/kg)^2. Now, Newtonian gravity is a classical theory and there is no such thing like a running G (although the situation might be different in alternative theories of gravity, such as scalar-tensor theories, but this is another story...). Indeed, G is a constant no matter how close the two masses are or how massive the objects are. In a quantum field theory, G would depend on the energy involved, for example on the typical distance of the interaction.

If you think about that, this is a beautiful and elegant concept: it teaches us there's no such thing like "the ultimate theory", but each theory (if consistently quantized) would be different at different energy scales. For example, a theory like electromagnetism (or QED in its quantum version) becomes more strongly coupled as the energy increases. The QED coupling constant (the fine structure constant α) is about α ≈ 1/137 at low energies, whereas one measures α ≈ 1/127 at the scale of the Z boson, about 90 GeV. A theory like quantum chromodynamics (QCD) behaves exactly in the opposite way and it becomes more weakly coupled at high energies. This phenomenon is called asymptotic freedom (because the interaction between particles becomes zero at infinite energy) and its discovery  (by Frank Wilczek, David Gross and David Politzer) was worth the Nobel prize in 2004.

What does this have to do with Scotland? (if anything...) The idea that can be borrowed from particle physics is that of a "running citizenship". In other words, each person changes her/his sense of belonging to some country/community accordingly to the "characteristic scale of the problem". It's something that European people are already experiencing given that economy in Europe is mainly governed on European scales, whereas local regulations are governed by state laws. Something similar also happens for federal countries, although the idea of running citizenship that i'm trying to describe has more to do with sense of belonging than with politics (politics often tries to change the sense of belonging and to tailor it accordingly, though).

In physics, the theory that studies the running couplings is called renormalization group and the running is usually called "flow". In most theories, the coupling either grows or decreases with energy, but for some special theories it asymptotes a constant value, a "fixed point".

As for the running citizenship, my impression is that we better try to have a fixed point for that, because the other two cases are quite catastrophic. The analog of a theory like QED would be a sense of citizenship that becomes smaller and smaller as smaller scales are approached, eventually terminating in individuals that do not belong any community. This would imply a sort of total isolation for each individual. The other case would be funny: an individual would become more and more aware of the global nature of Mankind and would feel like more and more part of the entire Universe as smaller scales are approached (this sounds like a nice outcome but perhaps a bit too Hippie for these times....). The most natural solution would be approaching a limit, a minimum size of the community (which we can perhaps identify with the family or hopefully with something larger than that) and then having each person feeling as a part of a larger community dependending on the context and the environment.

In which category does the running citizenship flow of the Scottish people fall? We shall discover this quite soon and the outcome has probably very little to do with physics.....


Sunday, August 31, 2014

Greetings from Mons

Some of the participants of the Mons Meetings 14 held this week at Mons, Belgium, and greatly organized by my colleague and friend Terence Delsate (the guy wearing glasses in the group picture...)

Tuesday, July 22, 2014

Jordi on Dark Matter @ FameLab 2014

Fame Lab is a competition to find new voices of science across the world. In these events various speakers compete for the best popular science short talk. The events are hosted in various countries and there are competitions at regional, national and international level.

This year Jordi Casanellas (former PhD student in IST-Lisbon and now postdoc at the Albert Einstein Institute near Berlin) attended Fame Lab Germany. As the video below shows, in the first stages of the competition speakers cannot use blackboards (not to mention slides or projectors) and their talk has to be ~3 mins long.



Jordi talked about his field of research, Dark Matter, and in fact did a great job: he passed the regional competition and went to the national finals (see video below), where he placed second!




So, if you want to have an idea of what Dark Matter exactly is (or what scientists actually think it should be...) you don't have to do anything but listen to Jordi's speeches. Enjoy!

Sunday, July 13, 2014

Pull back: "Scientist: Four golden lessons" by Steven Weinberg

Just came across this brilliant essay by Nobel Laureate Steven Weinberg, writing about his experience as a young scholar, his first steps in research and the connection between science and epistemology.



The essay is so short and clear that I could have copied it here in its entirety, but I'll just give you one inspirational paragraph:

[...]
Look back 100 years, to 1903. How important is it now who was Prime Minister of Great Britain in 1903, or President of the United States? What stands out as really important is that at McGill University, Ernest Rutherford and Frederick Soddy were working out the nature of radioactivity. This work (of course!) had practical applications, but much more important were its cultural implications. 
[...]

and leave the rest for the original

Sunday, June 8, 2014

Vita dura per i neutrini sterili e non solo



Si è appena conclusa a Boston la conferenza NEUTRINO2014 dedicata, così come vuole il nome, ai nuovi risultati sperimentali e teorici che provengono dal mondo di queste elusive e misteriose particelle, per l’appunto, i neutrini.

Ci sono parecchie novità interessanti e volevo quindi fare un piccolo riassunto sulle cose più sfiziose.

Partiamo dalla ricerca dei cosiddetti neutrini sterili, e cioè di quelle particelle ipotetiche che sono state introdotte per spiegare alcune anomalie riscontrate nel corso degli anni da alcuni esperimenti che non si inquadravano nel modello delle oscillazioni a tre neutrini. Il primo esperimento a riscontrare un’anomalia è stato LSND (Liquid Scintillator Neutrino Detector) a Los Alamos, in cui è stato registrato un eccesso di antineutrini elettronici, con significatività di 3.8 sigma, su un fascio pressoché puro di antineutrini muonici. Se interpretati in uno schema di oscillazione a due neutrini, per la particolare configurazione della baseline, L, (la distanza tra sorgente di neutrini e rivelatore) e l’energia, E, da cui dipendono la probabilità di oscillazione di un neutrino muonico ad uno elettronico \[ P_{\nu_{\mu}\rightarrow\nu_{e}}\left(L,\, E\right)=\sin^{2}2\vartheta_{e\mu}\sin^{2}\left(1.267\:\frac{\Delta m_{41\,}^{2}L}{E}\right) \] questo eccesso sarebbe indicativo di un'oscillazione con una piccola ampiezza e un grande \(\Delta m^{2}\sim1\) \(\textrm{eV}{}^{2}\). Appare chiaro che un \(\Delta m^{2}\sim1\) \(\textrm{eV}{}^{2}\), non può essere incorporato in un modello a tre soli neutrini (elettronico, muonico e tauonico) in cui esistono solamente due differenze di masse al quadrato indipendenti. Infatti deve valere la relazione \[\Delta m_{21}^{2}+\Delta m_{32}^{2}+\Delta m_{31}^{2}=m_{2}^{2}-m_{1}^{2}+m_{3}^{2}-m_{2}^{2}-m_{1}^{2}-m_{3}^{3}=0\,\] e dal momento che la differenza di massa al quadrato dei “neutrini solari” è \(\Delta m_{SOL}^{2}=\Delta m_{21}^{2}=7.58_{-0.26}^{+0.22}\times10^{-5}\) \(\textrm{eV}{}^{2}\) e di “quelli atmosferici” è \(\Delta m_{ATM}^{2}=\left|\Delta m_{31}^{2}\right|\simeq\left|\Delta m_{32}^{2}\right|\simeq2.35_{-0.09}^{+0.12}\times10^{-3}\) \(\textrm{eV}{}^{2}\), non vi è spazio per una differenza di massa al quadrato dell'ordine dell'\(\textrm{eV}{}^{2}\), se non in uno schema in cui sia presente almeno un nuovo stato di neutrino massivo \(\nu_{4}\) sterile, per cui possa essere interpretata la differenza di massa al quadrato come \(\Delta m_{\textrm{new}}^{2}\equiv m_{4}^{2}-m_{1}^{2}=\Delta m_{41}^{2}\). Questo neutrino però deve essere sterile, e quindi non deve partecipare a nessuna delle interazioni (tranne quella gravitazionale) in quanto esistono delle misure effettuate al LEP sul decadimento del bosone Z in neutrini, che indicano che il numero di neutrini “attivi” (e cioè quelli che interagiscono per forza debole) deve essere esattamente tre.