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Showing posts with label CMS. Show all posts
Showing posts with label CMS. Show all posts

Sunday, 20 December 2015

Friday wrap-up: diphoton excess, no diboson, no gluinos...

What a week! We have already seen some 40-odd papers submitted to hep-ph in the last few days on the "recent observed diphoton resonance" [1]. Well I certainly wouldn't go that far but ATLAS and CMS have each seen an excess of events in the diphoton spectrum at around 750 GeV, which is amazing since apparently they weren't even searching for it [2], and anyway beside the point because they also discovered a gluino [3]. Sloppy science writing aside, what do we know?...

  • The CMS and ATLAS Run II physics results presentations can be found here. Of course, all results presented are preliminary. The result that has hep-ph buzzing, though, is a little bump atop the falling diphoton invariant mass background (conference notes here and here). [See Jester, Motl, Strassler (here and here), PhysicsMatt, or Eilam Gross for some physicist perspectives. Else in popular media I thought the NY Times article was fairly balanced, but then I am a phenomenologist]. You can eyeball the bumps in question below (credit to Strassler for this image):


    But what about the numbers? The rumours were as accurate as one could reasonably ask: assuming a narrow width resonance, CMS observed a 2.6σ local (1.2σ global) excess at 760 GeV [increases to 3.0σ local (1.7σ global) at 750 GeV when combined with the 8 TeV data], and; ATLAS observed 3.6σ local (2.0σ global) at 750 GeV [have not yet combined with 8 TeV, but if they did it appears the significance would fall]. Allowing the width to float to larger values, the CMS result goes down to 2.0σ local, whereas ATLAS observes a best fit 45 GeV (6%) width at 3.9σ local (2.3σ with multivariate look-elsewhere). The relevant slides are below:


    It is a tantalizing excess. Sensibly, what one would like to know is the global significance of the fully combined (CMS+ATLAS 8+13 TeV) datasets. It is non-trivial to get an exact number (see here or here), but one can at least make a good bet that it's greater than about $\sim \sqrt{1.7^2+2.0^2}\approx 2.6\sigma$, perhaps in the vicinity of $\sim 3\sigma$. [I would imagine the demand for a joint analysis is high enough to be a priority for the collaborations (or they might try to avoid feeding the hep-ph sharks?), so maybe we will have that number by Moriond]. This being a (very rough!) ~1/300 chance then, and given the hundreds of plots CMS and ATLAS produce, it is very possible that this is just a statistical fluctuation. Nonetheless, this excess is being taken fairly seriously, and will be exercising our scrolling finger on hep-ph for the foreseeable future while we grapple with the sensible question: if it is real, then what could it be and what does it imply? The answer to this question may have implications for the experimental program of the LHC over the next few years (at least), and so phenomenologists are already relentlessly hard at work...

    So let's try to answer that question: what could it be? Well, there is no evidence for any extra activity in the excess events, so it appears consistent with a simple $gg\to X\to \gamma\gamma$ resonance. If taken as a resonance, the events translate to a cross-section $\sigma(pp\to X)\times Br(X\to \gamma\gamma)$ of $\sim 2$/fb ($\sim 6$/fb) in the narrow (wide) width scenario. Let us try to build a model with these properties. The simplest thing is to add a scalar singlet to the standard model. To couple it to gluons and photons let's borrow the Higgs' trick and couple it to some coloured/charged fermion(s) which then induce the couplings via a loop. Let's try Yukawa coupling it to a vector-like up-type quark first, write down the effective couplings, and calculate the Yukawa necessary; we find that it has to be huge ($\sim 5$ or so). And there's a potential problem, since the singlet will want to decay most of the time to the up-type quark. That's okay! We will just make it heavy enough (> 375 GeV) so that it's not allowed. Now we're done, and this solution is "already well-known" [4]. We can add more vector-like fermions to quell the large Yukawa(s) somewhat and/or dial the $gg$ and $\gamma\gamma$ couplings independently. If we take the large width seriously, we still have to add extra decay channels, and then dial up the production and/or branching to photons to compensate. The obvious options are a dark sector or some other standard model states, which we have to hide from previous searches. We could also try constraining ourselves inside some more predictive (restrictive) model.

    Of course there are several papers on just the above, the implication being that you need more than just the singlet scalar, which is obviously quite interesting. The immediate implications for the LHC are: look for anything at 750 GeV in $jj, Z\gamma, ZZ$ (in roughly descending order of promise) as soon as is possible.

    But this is just a minimal model. It could also be a scalar/pseudoscalar/bound state connected to compositeness/extended gauge group/extra dimensions/hidden valley/SUSY/dark matter/naturalness, and you can be sure there are already arXiv submissions on all of these. On that, it seems to me that arXiv isn't quite the ideal platform for all this. It would be nice instead to have all the various proposals in the same place, with the same formatting, in no-nonsense form, all grouped by some general properties. Then the interested phenomenologist/experimentalist could go and browse a list of, for example: (1) candidate; (2) production; (3) couplings; (4) decays; (5) associated activity; (6) additional particles; (7) additional predictions. Of course this will inevitably be done anyway by some authors in a review, but it seems like the same could be achieved much more efficiently with a community-run wiki or similar, as long as there were some moderators willing to dedicate their time to such a project... any thoughts on this from readers?

    In my book there's not much more to say except we need more data, to tell (1) if this is real, or (2) what it is. Looking forward to more excellent work from our experimental colleagues in the new year.

  • Now onto other matters from the presentation. First the diboson excess from Run I. Before the meeting a couple of useful papers appeared on the arXiv: a third-party CMS+ATLAS statistical combination, and; a thorough summary and literature survey. Now we know both CMS and ATLAS see nothing significant in Run II data (although they do not have sensitivity to conclusively probe the parameter space of interest):

  • Also in Run II data, the on-Z excess is not seen by CMS, but still persists at ATLAS...

  • As well, lots of gluino searches in different final states but nothing seen, and limits improve to roughly 1.2--1.8 TeV in the simplified models considered (but of course there are always compressed places to hide!).
  • CMS have not unblinded any of their Higgs analyses, but ATLAS reported results in γγ and ZZ: they were expecting 3.4σ observation and saw instead 1.4σ. Obviously the Higgs has packed up, moved to 750 GeV, and remembered its earlier proclivity for photons (this hypothesis will be robustly tested in upcoming LHC analyses).
  • Moving on to other news, LUX has released new limits on spin-independent dark matter nucleon scattering. See the press release and/or this blog post from Sally Shaw for a summary. They're almost observing solar neutrinos!

  • "NuPhys2015: Prospects in Neutrino Physics" was on this week (indico).
  • Links without thinks:
    • Strumia's insta-paper archive.
    • Quanta: "A Fight For the Soul of Science," on the recent meeting at the intersection of the philosophy of science and theoretical physics.
    • Quanta: "Landmark Algorithm Breaks 30-Year Impasse."
  • In audio/video media:

[1] arXiv: "The recent observed diphoton resonance around 750 GeV at the LHC..."
[2] Nature News: "... the 750 GeV boson is not one of the particles that LHC physicists have been searching for..."
[3] Tech Times: "Physicists Have Discovered Evidence Of A Gluino Particle, The Cousin Of The Higgs Boson."
[4] arXiv: "It is already well-known that a real singlet scalar ϕ with Yukawa couplings ϕXX to vector-like fermions X with mass mX>mϕ/2 can easily explain the observed signal, provided X carries both SM color and electric charge."


Saturday, 5 September 2015

Friday wrap-up: ATLAS+CMS Higgs combination, THE rankings...

Wherein I list some (mostly) recent happenings, ramble a bit, and provide links, in an order roughly determined by importance and relevance to particle physics. Views are my own. Content very definitely skewed by my own leanings and by papers getting coverage, and it may not even be correct. It is a blog after all...

  • Conferences of interest this week include The 3rd Annual Large Hadron Collider Physics Conference (LHCP2015; indico; twitter), and QCD@LHC 2015 (indico).
  • At LHCP, Marco Pieri presented the brand new ATLAS+CMS Higgs combination (talk here [pdf]). Slides 17 and 18 tell the story for the SM Higgs versus the null:


    The interesting things for me are: global signal strength fit is $\mu=1.09^{+0.11}_{-0.10}$, H→ττ and VBF production are (preliminarily) "discovered" at >5σ, and ttH has a mild (2.3σ) excess (already hinted at Moriond) to keep an eye on. Different parameterisations are also studied, finding, of course, everything consistent with a SM Higgs. Would imagine we can look forward to the arXiv paper soon.
  • The Times Higher Education World University Rankings have decided to exclude from their analysis all papers with more than 1000 authors for the 2015-16 rankings. This obviously has a big impact on those involved in the ATLAS/CMS collaborations. Interesting to read the comments below the post from John Ellis, James Stirling, and Andrew Hamilton, among others.
  • According to this nature news article, there are some concerns for the cooling pumps in the AMS-02 experiment. There were originally four cooling pumps. They write: "Only one pump is needed at any given time. One failed in February 2014 and at least one of the other three is showing possible signs of trouble." Also: "[Ting] exhibited little patience for questions about the cooling pumps. 'We have four pumps — we only need one,' he says. 'We expect to operate for the lifetime of the space station.'"
  • Some movement on the Hawking/Perry/Strominger proposal for the black hole information loss problem. There's now a short stake-claiming arXiv paper, and an hour-long talk from Malcolm Perry on YouTube. Sabine Hossenfelder reacts here.
  • From CERN: a summary on LHC Run 2 so far from Rolf Heuer (he comments on the CMS magnet: "... it’s clear that there are contaminants in the cold box that supplies the magnet with liquid helium, and this will therefore need a thorough clean.... All being well, CMS will be able to take data satisfactorily with field on until the end of the 2015 physics programme, postponing the cleaning operation until the winter stop in order to be ready for the start of 2016."), and a summary on recent scrubbing runs.
  • In video/audio media:
  • Lastly, here is an antineutrino global map: an experimentally informed model of Earth’s surface antineutrino flux over the 0 to 11 MeV energy spectrum.

Friday, 26 June 2015

Friday wrap-up: first physics, CMS magnet, diboson excess...

Wherein I list some (mostly) recent happenings, ramble a bit, and provide links, in an order roughly determined by importance and relevance to particle physics. Views are my own. Content very definitely skewed by my own leanings and by papers getting coverage, and it may not even be correct. It is a blog after all...

Long time no blog -- turns out to be hard to keep up with everything in the midst of travel. So here are some "links without thinks" from the last month...
  • As of June 3 the LHC has physics data being taken at 13 TeV! The live blog from the day can be found here [1 of 4], and there are five highlights videos on the CERN YouTube channel. The media hype for this milestone was significantly larger than for the first 13 TeV collisions 21 May. I wonder if this was a calculated decision from CERN... it seems that's what would have been preferred after the 7 TeV restart in 2010 (see Particle Fever e.g. 1:00:20).

    ATLAS made public a dijet animation and the below pp collision events with 17 vertices(!) from June 3...


  • There was a rumour a couple of weeks back that the CMS magnet was in trouble. The earliest article I am aware of is this one (dated 8 June), which with the help of Google Translate suggests oil contamination of the liquid helium involved in cooling the 4T superconducting magnet. You can read the immediate response of CMS physicists here. Now CMS has released a statement (14 June), which is partly quoted below.

    CMS has been taking collision data since the 13TeV startup of the LHC on 3 June. During this period, the CMS magnet has been kept off due to an issue with the cooling system... The issue with the magnet cooling system was identified in the final preparatory phase leading to collisions in the LHC. While preparing for beam in CMS, a problem was found in the system that feeds liquid helium to the CMS superconducting magnet. The problem was diagnosed to be due to oil, which is used in the initial compression stages, reaching the so-called 'cold-box’ of the cryogenic system. The cold-box is a complex system with several sets of filters protecting three turbines along the path of the helium towards the magnet. In order to clean the oil contamination essentially all components of the cold-box have been extracted and replaced... CMS is confident that, following the LHC technical stop and the beam conditioning run that will start at the end of this week, after the low-intensity and commissioning period, the full magnetic field will be available for the 13 TeV LHC run.
  • Certainly a month couldn't go by without another excess to keep people busy! Now it is in an ATLAS search for diboson resonances.


    The excess is of ~3σ local significance in WZ, WW and ZZ channels, and 2.5σ global. Jester has a write-up and some thoughts, and notes that there is a small excess at around the same mass scale in similar CMS searches. Along with the CMS WH resonance and right-handed W excesses at around 2 TeV, who knows, maybe there's life out there in the desert yet... and not too far away...

    (image credit John Pritchett)

    PS: I hear the ATLAS $h\to \mu\tau$ analysis is hopefully out within weeks (context)...
  • The OPERA experiment has observed (i.e. at 5σ significance) tau neutrino appearance in a muon neutrino beam.
  • The Perimeter Institute Convergence conference June 20-24 is archiving its very interesting talks here.
  • The CMB@50 Conference held at Princeton from 10-12 June has been "storified" by Renée Hložek, links at her blog.
  • In space news and pretty pictures:
    • The Philae lander on Comet 67P/Churyumov-Gerasimenko is awake again, and ready to do science...

      Landing
    • ... Pluto and Charon in colour from New Horizons...


      (Only a couple of weeks now until closest approach: “Color observations are going to get much, much better, eventually resolving the surfaces of Charon and Pluto at scales of just kilometers.”)

Friday, 15 May 2015

Friday wrap-up: IBL, SABRE...

Wherein I list some (mostly) recent happenings, ramble a bit, and provide links, in an order roughly determined by importance and relevance to particle physics. Views are my own. Content very definitely skewed by my own leanings and by papers getting coverage, and it may not even be correct. It is a blog after all...

  • ATLAS News had a wrap-up of the 900 GeV collisions performed last week. It was cool to see an event display with the insertable B-layer in action (the fourth and most inner layer of the pixel layers on the right insert):


  • The Stawell Underground Physics Laboratory project here in Australia has received $1.75 mil from the federal government to match the State's contribution from earlier this year. The funding will go a significant way to constructing the clean room to host SABRE, the first southern hemisphere dark matter direct-detection experiment, the advantages of which I've mentioned earlier.
  • If the dark matter distribution in M87 is spiked at the centre, then this arXiv preprint claims that thermal relic dark matter is ruled out for an unprecedented $m_{DM}\lesssim 100$ TeV! As well, an apparent excess at high energies can be explained by $\mathcal{O}(1-100)$ TeV dark matter. I wonder if this paper will become another galactic centre excess for hep-ph?
  • The result has been on the arXiv for a while, but the CMS+LHCb $B_s (B^0)\to \mu^+\mu^-$ analysis was published in Nature, which I thought was interesting enough to note. As far as I can tell from a quick Inspire search, this is the first paper from the LHC Collaborations published in Nature. Note the 6 months from receipt to publication...
  • A few very interesting articles this week:
    • Nautilus: the story behind the OPERA superluminal neutrinos.
    • Aeon: on the pervasiveness and apparent non-falsifiability of inflation.
    • Scientific American: on physicists as philosophers.
    • Quanta: ultra-high energy cosmic rays, the Oh-My-God particle, and an EeV+ hotspot in the sky.
  • In video/audio media:
    • New physics frontiers at the 13 TeV LHC from CERN. [3 minutes]
    • A first video spot at Quanta Magazine: In Theory with David Kaplan (of Particle Fever fame) on what happens if you fall into a black hole. [2 minutes]
    • And if you'd like to learn more about the man responsible for backing the foundation that supports Quanta Magazine in the first place (and for Chern-Simons forms, and for Renaissance Technologies), you should watch the very interesting interview with James Harris Simons at Numberphile. [19 minutes]
    • Stephen Hawking on intelligence. [15 minute talk]
    • Excellent video at SmarterEveryday on how the window shutters on the space station work. [8 minutes]
  • Finally, updates on space missions: 
    • New Horizons can now make out all of Pluto's known moons.

    • The bright spots on Ceres we've been following now appear to be deposits of ice at the bottom of a crater.




Friday, 27 March 2015

Friday wrap-up: LHC delay, B to Kμμ, Higgs at N3LO, dark matter self-interaction...

Wherein I list some (mostly) recent happenings, ramble a bit, and provide links, in an order roughly determined by importance and relevance to particle physics. Views are my own. Content very definitely skewed by my own leanings and by papers getting coverage, and it may not even be correct. It is a blog after all...

  • The LHC did not see a circulating beam this week due to a short circuit in one of the magnets, likely due to debris in a diode box. Delay could be days or months. Read the CERN press release here, and there's some more information at Nature News. [Edit: more from CERN here.]
  • The ATLAS/CMS combined Higgs mass measurement is now up on the arXiv (~6000 authors!).


  • There has been a bit more talk on the LHCb $B\to K^*\mu\mu$ excess which was updated from 1/fb to 3/fb of data last week. The Conf Note is now up. There's a short blog post on interpretation from David Straub, and the Straub/Altmannshofer Proceedings paper has quite a nice summary. See also the Resonaances post and the previous-two posts also there.

    Shown below is the old result (blue) and new result (black) against theory (orange) for the angular observable of interest.


    The point is that the 4--8 GeV^2 bins each deviate from the theory prediction, and a naive combination suggests a 3.7σ tension. This happens to be the same tension seen in the analysis with 1/fb, which suggests that the new data have still fluctuated up, but not quite as much. The effect has not gone away. But I am with Tommaso... I would like to know what is the probability of seeing such a deviation or larger in any of the angular observables they looked at, assuming the null. Probably this is difficult to do; likely there are significant correlations between bins of different observables(?)... still, it would be nice to know a number for the global significance as well.

    The question now is whether we are seeing new physics or underestimated theory uncertainty. The data are not suggesting any problem with form factors, but an unexpectedly large charm-loop contribution near $J/\psi$ is a possible explanation. If it is new physics, then the discrepancy can be explained by a single operator$$O_9=(\bar{s}\gamma_\mu P_L b)(\bar{l}\gamma^\mu l)$$quantified by a parameter $C_9^{NP}$. This could also go some way to explaining the 2.6σ deviation from lepton-flavour universality (quantified by $R_K$) also measured by LHCb. According to the Straub/Altmannshofer Proceedings there are sensible ways to proceed if we want to discover the culprit. Here are a few of them:

    1. Keep looking at q^2 dependence of $C_9$; the new physics effect should be q^2 independent.

    2. Measure $B\to K^*\mu\mu$ and $B\to K^*ee$ branching ratios and angular observables. If the same new physics is responsible for this and $R_K$ then you might see "spectacular" deviations.

    3. Search for lepton flavour violations in $B\to K^*\mu e$.

    Certainly these are all measurements to look forward to...
  • If you want more insight into what's going on at Moriond, their twitter stream is excellent.
  • There's another excess that you might see making the rounds soon. They're everywhere! This week it is >2σ in a search for WH resonances in $l\nu b\bar{b}$.


    Of interest are the three events at ~1800 GeV. It is only seen in the electron channel, so if it is new physics, it is not probably not a WH resonance. It is almost not worth mentioning, but CMS also saw an excess in their right-handed W search in $lljj$. There they saw a >2σ discrepancy in the electron channel at around the same mass scale.


    I have not had time to read about these in detail, but if they can be linked, they will be linked. Watch the arXiv...
  • Higgs gluon-fusion production cross-section has been computed at N3LO (and Moriond talk here [pdf]), "the first ever complete computation of a cross-section at N3LO at a hadron collider."
  • Hooper and Linden have weighed in on the Reticulum II gamma-ray excess (seen in one of the newly discovered DES dwarf satellites). From the conclusion: "In order for this excess to be compatible with the lack of significant gamma-ray detections from other dwarf galaxies (most importantly, Segue 1 and Ursa Major II), Reticulum II must contain a high density of dark matter... A measurement of Reticulum II’s J-factor that is much smaller than this value would place serious doubt as to any dark matter interpretation of its excess."
  • There was lot of hype relating to a lazy LHC article in the media this week. On the plus side, Backreaction has an excellent rebuke (on the article and the paper that spawned it), and there you can also learn a bit about rainbow gravity.
  • A paper published in Science used the Chandra and Hubble Space Telescopes to observe 72 galaxy cluster collisions and subsequently constrain dark matter self-interaction. This number now supersedes the constraint from the bullet cluster. You can read the press release or watch the astrophysicists involved (along with others) discussing it on YouTube [1 hour].

    Images of galaxy clusters
  • A paper appeared on the arXiv today, signed by a number of physicists from many different institutions, commenting that the Nature paper on inner galaxy dark matter appearing a month or so back was not even wrong: "Considerable confusion may stem from the use of the term ‘inner’. The Sun’s orbit encompasses roughly 90% of the stellar mass. By this standard, we live in the outskirts of the Galaxy. That some DM is needed interior to the Solar circle is neither surprising nor new."

Friday, 20 March 2015

Friday wrap-up: Higgs mass combination, ttH, LHCb rumour...

Wherein I list some (mostly) recent happenings, ramble a bit, and provide links, in an order roughly determined by importance and relevance to particle physics. Views are my own. Content very definitely skewed by my own leanings and by papers getting coverage, and it may not even be correct. It is a blog after all...

  • Long Shutdown (LS1) is over, and we should have the first fully circulating beam next week!

    You can track LHC and CMS status here and even view live events. CMS are currently doing their cosmic run with the magnet only turned up a couple of days ago; I managed to catch a nice one bending in the B field:


  • The ATLAS/CMS preliminary Higgs mass combination was presented for the first time at Moriond (talk here [pdf]). The result is $$m_H=125.09\pm0.24\, [\pm0.21\text{ (stat.)}\pm0.11\text{ (syst.)] GeV}$$

  • ATLAS has submitted their results on $t\bar{t}H$ production with $H\to b\bar{b}$ and released a Conf Note on $H\to WW,\tau\tau,ZZ$. Both see a small excess over the SM (of some interest only because CMS has $\mu_{ttH}$ at $>2\sigma$ above SM). I assume that those results enter into the following plot also presented in the Moriond talk(?). At least it is something to keep half an eye on in Run 2, while it likely goes away...


  • Also released for Moriond are new results on Higgs decays to dark photons: both $H\to\gamma_d\gamma_d\to 4l$ and $H\to Z\gamma_d\to 4l$ (talk here [pdf]). Nothing seen, but a nice result, especially looking into Run 2 when they are likely to explore significant parameter space for the Higgsed dark photon model.
  • There's a rumour (via Jester) that the LHCb $B\to K^*\mu\mu$ analysis for the full 3/fb of data is due out soon, and it confirms the anomaly already observed in the previous analysis. If it is today then that would line up with the heavy flavour day at Moriond. See these-two Resonaances posts for an easily digestible recap, or dig deeper with any of these...

    Edit: Now confirmed; significance $\approx 3.7\sigma$... see LHCb news and the talk slides [pdf]. Below is new result (black) and old result (blue). Conf Note out soon.


  • Super-Kamiokande has set the best limits on spin-dependent dark matter annihilating indirectly to neutrinos in the Sun.


  • Quanta Magazine has an interview with Steven Weinberg which touches on his view of the history of science and where it's at now, including some discussion on the multiverse.
  • In video/audio media:
    • Dancing in the Dark documentary on the LHC and dark matter is on BBC iPlayer for the next month or so [60 minutes], and a radio programme as well [43 minutes].
    • A video about the LHC from Fermilab featuring Don Lincoln. [6 minutes]
    • It was Super Pi Day last week... here is ViHart's anti Pi Day rant. [4 minutes]
    • Visualisation of today's upcoming eclipse from NASA Goddard. [2 minutes]
    • Hunting new craters on the moon, from NASA Goddard. [5 minutes]
  • NASA's Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft has observed two unexpected phenomena in the Martian atmosphere: an unexplained high-altitude dust cloud and aurora that reaches deep into the Martian atmosphere. No mention in the NASA release or the Nature News, but I wonder if perhaps they are seeing again the plumes that hit the news a few weeks back?

Friday, 13 March 2015

Friday wrap-up: ATLAS on-Z excess, CMS kinematic edge, new dwarfs, dark matter annihilation...

Wherein I list some (mostly) recent happenings, ramble a bit, and provide links, in an order roughly determined by importance and relevance to particle physics. Views are my own. Content very definitely skewed by my own leanings and by papers getting coverage, and it may not even be correct. It is a blog after all...

  • ATLAS released a preprint yesterday (submitted to EPJC), Search for supersymmetry in events containing a same-flavour opposite-sign dilepton pair, jets, and large missing transverse momentum..., that is interesting for two reasons.

    1. Remember the 2.6σ kinematic edge excess that CMS observed in their similar analysis originally released as a PAS in August last year? If not then see Tommaso Dorigo or Collider Blog for a summary... or don't, since ATLAS don't see any hint of it!

    2. They call CMS's excess, and then they raise, with a 3.0σ excess in a different signal region (SR). So let's talk about that...

    The search is for an on-Z opposite-sign same-flavour (OSSF) lepton pair + jets + MET. They are motivated by a gravitino LSP SUSY scenario with pair-produced gluinos which decay via $\tilde g\to qq\tilde\chi_1^0, \tilde\chi_1^0\to Z\tilde G$ (though it seems to me like something as simple as a vector-like quark could also work). Anyway, after typical preselection and requiring two OSSF leptons (if more than two are present they take the leading leptons), they define the on-Z signal region as: $$81< m_{l^+l^-}/\text{GeV}<101, \\ n_{jets}\ge2, \\ E_T^{miss}>225\text{ GeV,} \\ H_T>600\text{ GeV,} \\ \Delta\phi(jet_{12},E_T^{miss}>0.4,$$where $H_T$ is the scalar sum of the jet and lepton $p_T$ in the event, and the $\Delta\phi$ cut is designed to reject background from mismeasured jets faking large $E_T^{miss}$. And backgrounds are tough... $Z/\gamma^*+jets$ with mismeasured jets producing difficult-to-model instrumental $E_T^{miss}$ is potentially worrisome, but it is made negligible by the $\Delta\phi$ cut. Flavour-symmetric backgrounds (with a truth-level flavour ratio $ee:\mu\mu:e\mu$ of 1:1:2) from $t\bar{t}$, $WW$, single top, and $Z\to\tau\tau$ are dominant; they are estimated with a data-driven method using opposite-flavour data as a control region. Fake leptons are estimated from data.  Diboson, $t\bar{t}V$, $t\bar{t}VV$, and $t+Z$ are estimated from MC, making sure not to double count the flavour-symmetric component.

    The expected and observed number of events as a function of invariant mass in the dielectron and dimuon channels are shown below:


    For the sum of both channels the expected background is 10.6±3.2 with 29 events observed, which ends up corresponding to a 3.0σ excess.

    Now, CMS did a similar search in the on-Z SR in their paper and didn't see anything. So are the results consistent? It's possible. The CMS SR wasn't quite as tight as the one employed by ATLAS. After similar preselection, for an on-Z signal region defined as $$81< m_{l^+l^-}/\text{GeV}<101, \\ n_{jets}\ge2, \\ E_T^{miss}>200\text{ GeV,}$$CMS have an expected background of $\approx$ 87.3±12.1 with 72 events observed. So who knows, maybe if CMS demanded $H_T>600$ GeV they would see something too, or maybe not... 
  • The biggest news of the week comes from Tuesday's astro-ph listings. This is not my area, so I can't comment intelligently, but anyone can read an abstract and look at Figures, so I will just sum up here for completeness and convenience (click the figures to make them larger)...

    1. Fermi-LAT released their Pass 8 constraints on dark matter annihilation (already largely known from preliminary results). They rule out dark matter masses $\lesssim 100$ GeV for a thermal relic annihilating to $b\bar{b}$ or $\tau\tau$. Those results are cutting into the best fit regions for the galactic centre excess.


    2. The Dark Energy Survey (DES) Collaboration has located eight new dwarf satellite galaxy candidates (of the Milky Way and/or Magellanic Clouds), and an independent Cambridge group has located nine using the publicly released DES deep photometry data. You can read the press release here.



    3. The new satellite candidates are prime spots to look for dark matter annihilation... so Fermi-LAT went and did it already! Assuming that the new candidates are dwarf spheroidals, they set a limit on the annihilation cross-section that rivals their Pass 8 results with known dwarfs above.


    4. But the story isn't over yet, because an independent group (which includes the Cambridge group that found nine candidates) has reported a gamma-ray excess, consistent with DM annihilation, in one of the new dwarf candidates. [Edit: The candidate is Reticulum II or DES J0335.6−5403, the green line in the above Fermi-LAT plot, which appears by eye to be the only line of all the candidates to have a weakened limit in the 10−few×100 GeV DM mass region, the region that would produce the excess.]


    And the dark matter annihilation saga continues...
  • Protons bunches half-circled the LHC beam pipe last weekend for the first time since the long shutdown began! Injector tests sent bunches from the SPS into the LHC ring and through ALICE and LHCb on their way to beam dumps. Both ALICE and LHCb recorded splash events when the beam was made to collide with a target.


    You can play with the LHCb event here. First fully circulating beam is expected at the end of the month.
  • PRL has published the Planck/BICEP2/Keck joint analysis, along with a Viewpoint article which tells some of the story -- we are reminded of the following: "... alternative models may be detectable with the next generation of experiments, some of which claim a sensitivity to r as small as 0.01. The competition is fierce, with at least six funded ground-based experiments underway (including the third version of BICEP), several balloon-borne experiments, and a number of proposed space missions."
  • There's a nice feature at ScienceNews about the AMS experiment, the positron excess, and Samuel Ting; on the (unreleased) preliminary antiproton data he remarks: "intriguing".
  • Published in Nature yesterday, the Cassini orbiter has detected tiny rock grains emitted from the plumes of the Saturnian moon Enceladus, hinting at a subsurface ocean. You can read the articles at NASA, ESA, or Scientific American. Meanwhile a team using Hubble have used observations of aurora to indirectly suggest that there is a subsurface ocean on Ganymede, Jupiter's largest moon. Nice to see that there are complementary ways to measure these things.
  • Today Rosetta is trying to listen for a signal from the Philae lander on Comet 67P/Churyumov-Gerasimenko. ESA released a cartoon video about it a few days ago [3 minutes]. The Lander Project Manager says, "It will probably still be too cold for the lander to wake up, but it is worth trying."

Friday, 13 February 2015

Friday wrap-up: Planck, long-lived particles, dark matter, neutrinos...

Wherein I list some (mostly) recent happenings, ramble a bit, and provide links, in an order roughly determined by importance and relevance to particle physics.

  • As for the rest 2015 Planck release, the base cosmological parameters have hardly changed (see e.g. Table 1 of this paper). ΛCDM of course continues to explain everything extremely well. The $\Sigma m_\nu$ upper limit is down to 0.17 eV (Planck TT, TE, EE+lowP+BAO) at best, almost at a level to rule out an inverted hierarchy ($\Sigma m_\nu\gtrsim 0.1$ eV). $N_{eff}$ is still at 3.04 ± 0.18 (Planck TT, TE, EE+lowP+BAO), consistent with the standard value 3.046. There is no longer a hint of an excess there. As for inflation, Jester weighed in, and Planck present their results in this paper:


    Looks like the canonical Starobinsky $R^2$ inflation (1980) is taking the lead, but time will tell... experiments will need to probe at the level r~0.001 to test it.
  • BaBar released a new paper, "Search for Long-Lived Particles in e+e− Collisions". No significant signal is observed. It seems worth mentioning that they see a high local significance of events in the dimuon mode at $m_{\mu\mu}\approx 212$ MeV, which interestingly is very close to the HyperCP anomaly, but they say it is consistent with background from photon conversions. Anyway, from the point of view of a phenomenologist I especially like the effort BaBar has put into presenting their results in a model independent way. For example:

    1. They provide upper limits on $\sigma(e^+e^-\to LX)\mathcal{B}(L\to f)\epsilon(f)$, where $L$ is the long-lived particle and $f$ is the final state, which are completely agnostic of the production mechanism.
    2. They provide limits on $\mathcal{B}(B\to LX_s)\mathcal{B}(L\to f)$ where $X_s$ is "strange stuff", which reduces significantly some theoretical uncertainties for exotic $B$ decays and increases the possible signal yield.
    3. They look at six different two-body final states.
    4. On top of this, they will provide the full efficiency as a function of $m$, $c\tau$ and $p_T$ in supplementary material, so that their results can be reinterpreted.

    Very well done from BaBar. Their measurement has implications for a very simple extension of the Standard Model with a real singlet scalar mixing with the Higgs (a Higgs portal). I have quickly reinterpreted their Fig. 3 bounds (1 cm < $c\tau_L$ < 100 cm) on the $\mu^+\mu^-$, $\pi^+\pi^-$ and $K^+K^-$ final states, assuming the limit lines are $\mathcal{B}(B\to LX_s)\mathcal{B}(L\to f)\lesssim 10^{-6.5}$...



    The above plot shows exclusions (within solid lines) for the model as a function of light scalar mass and mixing (see a previous paper of ours). The incremental shadings represent different lifetime regions and the shaded region between 0.28 GeV and 4 GeV masses indicates a very uncertain region for branching predictions; between we choose the most recent calculation (still >20 years old!) below 1.4 GeV and a perturbative calculation above. The approximate exclusion from BaBar is shown as the purple dashed line. Indeed they are exploring previously unexplored parameter space of interest for an inflationary model of Bezrukov/Gorbunov (between black dashed lines). They are limited by difficult backgrounds between 0.37 GeV and 0.86 GeV masses. The purple dotted line indicates the region they would have excluded if they could limit $\mu^+\mu^-$ and $\pi^+\pi^-$ final states to the same level in that region. 
    I am interested to get my hands on the supplementary material when it is released.
  • A new paper published in Nature Physics (not on the arXiv [edit: now it is]) this week is doing the rounds; it infers that there must be dark matter in the inner region (within the solar circle) of our own galaxy. It's behind a paywall, but there is a press release here. The main plot is below.

                      

    The authors have compiled an exhaustive list of rotation curve measurements (red), as well as gathered a set of models for the baryonic contribution from which they form their "baryonic bracket" (grey). The lower panel shows that all baryonic-only models are already ruled out at 5-sigma by the time we arrive at our galactic radii. Hence there must be a dark matter component in the inner Milky Way. They do not appeal to any dark matter density profile, so in that sense it is a model-independent result (but of course it is not independent of the baryonic models!). Nevertheless you can see that a typical Navarro-Frenk-White profile models the residuals extremely well. This is nice to know.

    It is interesting that you can already infer dark matter just with measurements of the rotation curve within the solar circle, and I suppose the result may also be useful to constrain dark matter distributions of interest to direct and indirect detection. I do not think it is "the first observational proof of the presence of dark matter in the innermost part of the Milky Way" as the press release claims (the paper does not claim this). It is obvious that you need some dark matter component in the Milky Way to explain the rotation curve measurements at large galactic radii, and nobody thinks that all that dark matter is accumulated beyond 8 kpc! Those measurements are already observational evidence for dark matter in the inner Milky Way. Regardless, Hooper et al. already saw dark matter at the galactic centre...
  • IceCube have released their results on the flavour ratio of astrophysical neutrinos above 35 TeV. They release a very nice plot which fits the observed flavour ratio at Earth:


    Averaging neutrino oscillations over astronomical distances would give a value in the blue triangle for any flavour ratio at the source. The blue circle $\approx(1:1:1)_{Earth}$ marks the expected value for pion decays as the dominant source. Any measurement inconsistent with the (very thin) blue triangle would be a signal of new neutrino physics, such as neutrino decay, sterile neutrinos, or CPT violation (see for example here and here). Tommasso discusses it a little more here. [Edit: there is a short article at the IceCube web site also.]
  • If you'd like to read some more on the "Firewall Phenomenology with Astrophysical Neutrinos" paper that appeared on hep-ph last week, Bee at Backreaction has written a nice summary. The paper shows that IceCube's PeV neutrinos could be explained by a suitable emission spectra from black hole firewalls.
  • CMS is alive! Magnet comes on next week.
  • Physicist Val Fitch, whose discovery (along with James Cronin) of CP violation in a 1964 experiment won him the 1980 Nobel Prize, has died at the age of 91. Read about his life and contributions here.
  • Steven Weinberg has written a history book, released a few weeks ago. According to the About, "To Explain the World is a sweeping, ambitious account of how difficult it was to discover the goals and methods of modern science, and the impact of this discovery on human knowledge and development." For some reason it even garnered praise from Ian McEwan.
  • IPMU has recently published a 26 page transcript [pdf] of a conversation with Edward Witten after he was awarded a Kyoto Prize last year for "Outstanding Contributions to the Development of Mathematical Sciences through the Exploration of Superstring Theory". Peter Woit highlights some excerpts and talks about it on his blog.
  • This blog post has a gif showing the history of planet detection in 1 minute, and the exoplanet gold rush starting at the year ~2000, with some discussion. Here's where we were by the end of last year:

  • On fake academic journals and "Rogeting".
  • SpaceX launched the Deep Space Climate Observatory (DSCOVR) on Wednesday. You can watch the launch and read a little about it at space.com. DSCOVR will sit at the L1 Lagrange point between the Earth and the Sun, observe the climate, and serve as an early alert "buoy" for geomagnetic storms. The satellite is the resurrection of a previous project championed by Al Gore; he wrote, "DSCOVR has embarked on its mission to further our understanding of Earth and enable citizens and scientists alike to better understand the reality of the climate crisis and envision its solutions. DSCOVR will also give us a wonderful opportunity to see the beauty and fragility of our planet and, in doing so, remind us of the duty to protect our only home."
  • Finishing up with some photos from space for the week:
    • Rosetta took an incredible shot of its comet. Tomorrow it will make its closest approach yet at 6 km above the surface, the Sun at its back.

      comet
    • Lastly, here is an image of galaxies SDSSCGB 8842.3 and SDSSCGB 8842.4 as pictured by Hubble and released on Monday