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Violation of CSI from two $\ell_a\neq\ell_b$ vortices. Never everywhere, always somewhere:
In the plane of radial contrast and angular separation, the CSI is satisfied in a band around equal radii, $r_1=r_2$, whose width oscillates with the angle between zero and a factor $(3+2\sqrt2)^{1/||\ell_b|-|\ell_a||}$ in $r_2/r_1$, and are violated everywhere outside this band. No choice of charges removes the band: $|\ell_b|\neq|\ell_a|$ implies $\ell_b\neq\ell_a$, so the relative phase always reaches $\pi$ somewhere, which fights violation. The band narrows with increasing $\big||\ell_b|-|\ell_a|\big|$.
Working on Violation of Cauchy-Schwarz Inequalities in Space and Time, I realize that the infamous $g^{(2)}$<1/2 criterion might have some sound meaning in violations of CSI inequalities with a thermal field as a reference, as opposed to a coherent one, which gives the antibunching scenario. If using another reference $b$, then CSI violations read: $$g^{(2)}_{aa}<\frac1{g^{(2)}_{bb}}\,.$$ Have $b$ thermal, you get $g^{(2)}_{aa}<1/2$. It doesn't make the criterion any better, except that such fields—still not being single-photon source ones—are able to violate CSI in an environment where standard fluctuations are the thermal ones.
Francis Halzen got the 2026 Nobel prize in physics, for IceCube and the discovery of astrophysical neutrinos.
I like to find the connection I have to every Nobel prize awarded. This year, this is to be found in our Referee reply to the Two photons everywhere[1] paper, where the Referee was complaining that something rare, even if big, is not significant. He wanted to rob us of my title and have it read "Two-photon correlations everywhere" instead. I told him "how about IceCube?" I didn't tell him "this'll get the Nobel prize in a couple of years" but could have:
Of course, the authors are the first to be aware that a correlated photon pair consists of two individual photons and that strong bunching at vanishing intensity does not imply that a relevant rate of photon pairs is available. Instead, it follows from strong bunching that two-photon correlations occur much more frequently than predicted by the Poisson statistics. Thus, for a sufficiently small intensity, one correlated photon pair per year can correspond to a value of g^(2) of 10^5. The authors will agree with me that from a practical point of view, i.e. in the presence of finite detection noise and with applications in mind, it is not justified to list such a region of the two-photon spectrum under the title "Two photons everywhere". I therefore suggest that the authors adapt their presentation in such a way that even an uninformed reader will not be misled.One of the points we wish to highlight is precisely that two-photon physics (multiphoton physics in general) is not related to the amount of signal, which is one-photon physics (or classical physics). Whether two-photon phenomena are, or are not, useful from a practical point of view is a secondary concern at our present level of description. We want to attract instead attention on the two-photon spectrum structure, with its two-photon Mollow triplet (of two-photon leapfrog transitions), circles of antibunching, unconventional bunching in the detuned Heitler regime, etc. All this is happening in the abstract two-photon space, which is not directly visible, but exists nonetheless, with no (theoretical) concern for signal. In this context, does one correlated-photon pair per year, to take the extreme case of the Referee, make a phenomenon unphysical? The IceCube collaboration recently reported the observation of seven (7) events in a 1 km$^3$ detector measured over the course of 10 years [Phys. Rev. Lett. 132:151001 (2024)]. The present text is, conceptually, at this level of description. In the two-photon spectrum, one does not need to—indeed, should not—refer to intensity: the structure exists regardless of the one-photon brightness.
What I couldn't tell him, of course, is that there were 124 people before the one guy who would get the prize (and he was in the top list):
For most people not from the neutrino community, that is the most obvious thing to comment upon: Halzen got the prize alone. The last one was Charpak in 1992. Before him, De Gennes (also French) also got it alone. For many physicists I know, a single awardee is a first time in their life. Since Cecil Powell in 1950, and Yukawa before him (the one after whom an institute is named in Kyoto), it is indeed more common to award various physicists. Before that, couples were the exception, even when such couples were Schrödinger and Dirac. The only triplet for the first 55 years of the prize was Becquerel and the two Curie, who were really one. Times change.
Wilhelm Conrad RöntgenHendrik A. Lorentz
Pieter ZeemanHenri Becquerel
Pierre Curie
Marie CurieLord RayleighPhilipp LenardJ.J. ThomsonAlbert A. MichelsonGabriel LippmannGuglielmo Marconi
Ferdinand BraunJohannes Diderik van der WaalsWilhelm WienGustaf DalénHeike Kamerlingh OnnesMax von LaueWilliam Bragg
Lawrence Braggnot awardedCharles Glover BarklaMax PlanckJohannes StarkCharles Edouard GuillaumeAlbert EinsteinNiels BohrRobert A. MillikanManne SiegbahnJames Franck
Gustav HertzJean Baptiste PerrinArthur H. Compton
C.T.R. WilsonOwen Willans RichardsonLouis de BroglieSir Chandrasekhara Venkata Ramannot awardedWerner HeisenbergErwin Schrödinger
Paul A.M. Diracnot awardedJames ChadwickVictor F. Hess
Carl D. AndersonClinton Davisson
George Paget ThomsonEnrico FermiErnest Lawrencenot awardednot awardednot awardedOtto SternIsidor Isaac RabiWolfgang PauliPercy W. BridgmanEdward V. AppletonPatrick M.S. BlackettHideki YukawaCecil PowellJohn Cockcroft
Ernest T.S. WaltonFelix Bloch
E. M. PurcellFrits ZernikeMax Born
Walther BotheWillis E. Lamb
Polykarp KuschWilliam B. Shockley
John Bardeen
Walter H. BrattainChen Ning Yang
Tsung-Dao LeePavel A. Cherenkov
Il´ja M. Frank
Igor Y. TammEmilio Segrè
Owen ChamberlainDonald A. GlaserRobert Hofstadter
Rudolf MössbauerLev LandauEugene Wigner
Maria Goeppert Mayer
J. Hans D. JensenCharles H. Townes
Nicolay G. Basov
Aleksandr M. ProkhorovSin-Itiro Tomonaga
Julian Schwinger
Richard P. FeynmanAlfred KastlerHans BetheLuis AlvarezMurray Gell-MannHannes Alfvén
Louis NéelDennis GaborJohn Bardeen
Leon N. Cooper
Robert SchriefferLeo Esaki
Ivar Giaever
Brian D. JosephsonMartin Ryle
Antony HewishAage N. Bohr
Ben R. Mottelson
James RainwaterBurton Richter
Samuel C.C. TingPhilip W. Anderson
Sir Nevill F. Mott
John H. Van VleckPyotr Kapitsa
Arno Penzias
Robert Woodrow WilsonSheldon Glashow
Abdus Salam
Steven WeinbergJames Cronin
Val FitchNicolaas Bloembergen
Arthur L. Schawlow
Kai M. SiegbahnKenneth G. WilsonSubrahmanyan Chandrasekhar
William A. FowlerCarlo Rubbia
Simon van der MeerKlaus von KlitzingErnst Ruska
Gerd Binnig
Heinrich RohrerJ. Georg Bednorz
K. Alex MüllerLeon M. Lederman
Melvin Schwartz
Jack SteinbergerNorman F. Ramsey
Hans G. Dehmelt
Wolfgang PaulJerome I. Friedman
Henry W. Kendall
Richard E. TaylorPierre-Gilles de GennesGeorges CharpakRussell A. Hulse
Joseph H. Taylor Jr.Bertram N. Brockhouse
Clifford G. ShullMartin L. Perl
Frederick ReinesDavid M. Lee
Douglas D. Osheroff
Robert C. RichardsonSteven Chu
Claude Cohen-Tannoudji
William D. PhillipsRobert B. Laughlin
Horst L. Störmer
Daniel C. TsuiGerardus 't Hooft
Martinus J.G. VeltmanZhores Alferov
Herbert Kroemer
Jack KilbyEric Cornell
Wolfgang Ketterle
Carl WiemanRaymond Davis Jr.
Masatoshi Koshiba
Riccardo GiacconiAlexei Abrikosov
Vitaly L. Ginzburg
Anthony J. LeggettDavid J. Gross
H. David Politzer
Frank WilczekRoy J. Glauber
John L. Hall
Theodor W. HänschJohn C. Mather
George F. SmootAlbert Fert
Peter GrünbergYoichiro Nambu
Makoto Kobayashi
Toshihide MaskawaCharles K. Kao
Willard S. Boyle
George E. SmithAndre Geim
Konstantin NovoselovSaul Perlmutter
Brian P. Schmidt
Adam G. RiessSerge Haroche
David J. WinelandFrançois Englert
Peter HiggsIsamu Akasaki
Hiroshi Amano
Shuji NakamuraTakaaki Kajita
Arthur B. McDonaldDavid J. Thouless
F. Duncan M. Haldane
J. Michael KosterlitzRainer Weiss
Barry C. Barish
Kip S. ThorneArthur Ashkin
Gérard Mourou
Donna StricklandJames Peebles
Michel Mayor
Didier QuelozRoger Penrose
Reinhard Genzel
Andrea GhezSyukuro Manabe
Klaus Hasselmann
Giorgio ParisiAlain Aspect
John Clauser
Anton ZeilingerPierre Agostini
Ferenc Krausz
Anne L’HuillierJohn J. Hopfield
Geoffrey HintonJohn Clarke
Michel H. Devoret
John M. MartinisFrancis Halzen