Of Particular Significance

Author: Matt Strassler

[NOTE ADDED: Unfortunately, within two months of this post, Mr. Zakaria was suspended from his job for plagiarism.  Such a spectacular lack of integrity calls into question everything he has ever written, and so I cannot anymore recommend his article, nor will he ever be quoted on this website again.]

 

Today I’d like to call your attention to an article by Fareed Zakaria, entitled “How government funding of science rewards U.S. taxpayers.”  (The sentiment also applies to taxpayers elsewhere, of course.) I can’t vouch for the details inside the article, but the point that Zakaria makes is one that I personally feel is very important.

When I give public talks about the fundamental research that I or my colleagues are doing, I am often asked, “what are its benefits to society?”  It’s a completely fair question, but with fundamental research it is typically far too early to know the answer; it can be many decades before the benefits, if any, become evident.  I think the best answer requires a long view — the kind of view Zakaria lays out in the article.  I often reply this way: that you should think about government investment in fundamental scientific research as similar to venture capital investments in many small startup companies; most of these efforts will fail, or will succeed with a small payout, but one or two will pay off in spectacular fashion and change the world.

And you surely want that payout to happen in a friendly country.  Zakaria  points out the worrying slope that the United States is on; though scientific breakthroughs have a big impact on the economy over the long term, funding for science is on a long-term decline (as a fraction of GDP) in the United States, while it is sharply increasing in a list of countries that include some that are not friendly to the United States.

Zakaria focuses on what is happening today in biotechnology, genetics, genomics, etc.  He also mentions the historical case of the transistor, the device that lies at the heart of our computer-based society. This last is an even nicer example if you expand your view.   The research that was done in the late years of the 19th century on the emission of light by atoms and on the electron led eventually to the equations of quantum mechanics, which in turn were essential in the development of the transistor.  No 19th century scientist could have predicted that the discovery of the electron would help put a cell phone in your pocket.

[Thanks are due to Leonid Kruglyak for bringing this article to my attention.]

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON June 22, 2012

[UPDATE: in the comments below, Dennis Overbye (the article’s author) explains what his wording was intended to imply, and that his article contains no error, just wording that was perhaps a little too simple.  I have also replied, with a request for much greater clarity in future, and explaining why I feel this is such an important issue.]

The New York Times has an article about the search for the Higgs particle! (Using the scientific jargon of physicists, it calls this particle the Higgs “boson”. If you want to know what a boson is, click here.)

Although a lot of the article is pretty good (though I can’t vouch for its accuracy in describing what’s going on inside the experiments) it does contain a HUGE conceptual and factual error that is vastly misleading.  [According to the author Dennis Overbye, this is not an error, but phraseology that is perhaps not entirely clear; see his comment below.] Here’s what it says about the Higgs particle:

“The new data will show whether [the hint in the December data] was a fluke or whether they are really on the road to discovering the long-lost [Higgs] boson, physicists say. They are racing to make a deadline to report the results at the International Conference on High Energy Physics, or Ichep, in Melbourne, Australia, starting July 4.

This, all agree, is the boson’s last stand. If the December signal fades, it probably means that the Higgs boson, at least as physicists have envisioned it for the past 40 years, does not exist, and that theorists have to go back to their drawing boards.”

This is misinformation — completely wrong — and in the interest of its readers, I do hope the Times would publish a correction.  [Again, I refer you to Overbye’s comment.]

This is NOT “the boson’s last stand”, and NOBODY agrees that it is the case.  What everyone agrees (with one caveat about heavier Higgs particles that actually haven’t been ruled out yet) is that it is the last stand of the Standard Model Higgs particle.   The Standard Model Higgs particle is only the SIMPLEST possible type of Higgs particle. Read about this form of Higgs particle here, if you like.

Let me say that again.  There is a big difference between ruling out the Standard Model Higgs particle and ruling out all possible forms of the Higgs particle.

Unfortunately, I’ve previously had to criticize the New York Times on precisely this point … back in August 2011.

Not finding the Standard Model Higgs particle — in Phase 1 of the Higgs search — just means that Phase 2 of the Higgs search has to involve a wider set of search strategies.  The two phases of the Higgs search was one of the main topics of my Cosmic Variance guest-post article and of this slightly more detailed article (both articles a bit out of date now as far as the data, but the basic point about the two phases still holds).  And in fact I pointed out in a related article, linking to some scientific lectures I gave on the topic, that it will take ten years to be confident there is no Higgs particle of any type.  I’m not telling you anything radical; ask any theorist in the field who has worked on Higgs physics and they will tell you the same thing.

So to say that “theorists will have to go back to their drawing boards” if the Higgs does not show up by December 2012 is badly mistaken.  There are hundreds of theory papers, going back decades, on versions of the Higgs particle (or particles) that would not show up by December 2012.   Here are some examples of such papers by well-known authors: http://arxiv.org/abs/hep-ph/0009158 ; http://arxiv.org/abs/hep-ph/0608310 ; http://arxiv.org/abs/1012.1316; there are plenty of such papers from the 1990s and even the 1980s.  Heck, I even wrote some myself.

One other minor error, caused by out-of-date information: the discrepancy between the masses of the possible Higgs signal seen at ATLAS and at CMS (which made the statistical combination of the two data sets unstable to small shifts) did indeed shift when the CMS data was reanalyzed in March.  The shift went in the “right direction”, eliminating the discrepancy and increasing confidence in the consistency of the ATLAS and CMS results.  On the other hand, the significance of the signal seen at ATLAS and CMS went down in March, too.  A complicated story; but these details won’t matter in the long run.

Of course, all of this may be moot, if more evidence for the Higgs shows up at the ICHEP conference in July.  But please, NY Times, get your facts straight on this very important point, which lies at the heart of the LHC program!  No discovery of the Higgs particle in 2012 absolutely will not mean that we know there is no Higgs particle at all.   It just means we would give up on the simplest version of the Higgs (which would be great news!), and that the Higgs search would move on to Phase 2.

Simplified diagram of how the Higgs search proceeds at the LHC; 2012 will be the transition point between Phase 1 and possible branches of Phase 2.
Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON June 21, 2012

Quick post today:

First, there were rumors about the Higgs particle search on Monday that got a lot of attention.  Caveat emptor: the experimentalists can’t possibly have their data in presentable form yet, so the rumors can’t be correct in every detail.   But if you are interested in a reasonable analysis of what the rumors would roughly mean if they were roughly correct, click here.  (I don’t personally see the point of doing lots of detailed analysis based on incomplete information, so if that’s what you want, I’m afraid you’ll have to find that on other blogs.)

Second, I’m still working on my sequence of extra dimensions articles; I’ve been working on a new one that explains what we can learn from Newton’s law of gravity (and Coulomb’s law for electric forces.)  This article is still a bit preliminary (still needs a very careful proofread) but if you’re interested you can take a look and comment on what you find confusing.

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON June 20, 2012

The rumors about the Higgs particle at the Large Hadron Collider [LHC] have begun again, and since that’s all anyone is going to want to talk about until we actually get the news for real, at the ICHEP conference in Melbourne in a couple of weeks, we may as well get started.

[This is especially true since we learned last year that some well-known non-particle-physicist bloggers have information pipelines directly into the experiments.  It is perhaps inevitable that there are scientists who see it in their best interest to subvert the scientific process.]

The current hot rumor is that the LHC experiments ATLAS and CMS have seen, in the new 2012 data, very roughly what they saw last December in the 2011 data, at least as far as the signal from a Higgs decaying to two photons (particles of light) in the mass range of 125 GeV/c2.  Note I am just repeating what I have seen on other blogs; as a matter of policy, I do not report secret information on this website, and I make no comment on the validity of any rumors.

Suppose this were true; what would it mean?  Well, it’s pointless to try to speculate about exactly how many standard deviations you would obtain by combining data in various ways — if I tried, the only thing I could guarantee you was that I’d get it wrong.  So rather than kick arbitrary numbers around based on guesswork, let’s talk about the larger picture.

There are two ways to think about the 2011 and 2012 data. One is to think about them as data sets you should combine together to extract the maximum information.  That’s what you would ideally do if you had access to all of the data and knew all the subtleties about how to do this.  It is not going to be that easy. Among many issues, one is that the data are taken at different energies, 8 TeV per proton-proton collision this year versus 7 TeV last year.  So in combining them you are making a theoretical assumption about how the production rate for Higgs particles changes as you change the energy from 7 TeV to 8 TeV.  That’s something you may or may not want to do, and at best it makes things rather complicated when you try to interpret the result.

Another way to think about it, as I discussed last week — and I think this will turn out to be more useful as a rule of thumb — is that last year’s data was good for excluding the Standard Model Higgs particle over much of the range for its mass that was available before 2011.  From a range of 115 to 800 GeV/c2 we’re now down, after 2011, to a range of something like 120 to 128  (where we can argue about the edges, but it doesn’t matter very much) or above 600.  The hints we saw last year at around 125 GeV/c2 (see also here, here and here) were very interesting and suggestive, but weren’t convincing, in part because with such a large range of possibilities to explore, the possibility of such hints appearing by random chance was not that low.  That’s due to the so-called “look-elsewhere effect”.  One could only obtain high significance by combining lots of different low-significance measurements together, a technique which can be very problematic, especially when some of these measurements are very difficult.

Now we come to 2012.  The LHC experiments ATLAS and CMS have just about the same number of collisions so far in 2012 as they had in all of 2011; and since the energy is a bit higher, the production rate for Higgs particles should be a bit higher (by several tens of percent.)  So what we’re going to see in the current 2012 data is a bit like a do-over of 2011… except that now the range of possible Higgs masses that needs to be explored is much smaller.  The smaller range means that if the same hints were seen in the same place as they were seen in 2011, the probability of this happening in the search region by random chance would be much lower than in 2011.  More precisely, this means the difference between the naive significance of any excess in the data, and the significance after accounting for the look-elsewhere effect, will not be very important.  Look-elsewhere was a big effect in 2011; but after the 2011 results, it will not be a big effect in 2012.  Thus (roughly) if you view the 2011 data as needed to narrow down the search region to a small window, you can roughly take the significance of any reported 2012 excess almost at face value.

So suppose we did see hints in the 2012 data that roughly resemble those in the 2011 data?  Then I think you’ll see most everyone agree that the evidence for something real in the data is pretty strong.  Of course we’ll need to see this in both the ATLAS and CMS experiments to have full confidence, but let’s assume that’s the case.  What would be next?

  • First, is what’s being seen in the data a Higgs particle at all?  Could it be something else?
  • Second, if it is a Higgs particle, is it the simplest possible type of Higgs particle — the Standard Model Higgs particle — or is it something more complicated?

I’ve described in some detail previously the strategy used to answer these questions, so I refer you to that article.

Generally, I suspect that the July 2012 data won’t be enough (even if you did try to combine it with the 2011 data) to shed clear light on these questions.  But the strong theoretical prejudice on the first question will clearly be that “what’s being seen is a Higgs particle of some type”; after all, the theory of the weak nuclear force requires there be something Higgs-like somewhere, and the Higgs in this mass range was predicted to show up first as a bump in the two-photon search.  I don’t think you’ll find many people who will think it likely that it’s not a Higgs particle, though due diligence will of course be needed to make sure.

The theoretical prejudice on the second question is much weaker, however; we really have no idea whether the Higgs is of Standard Model type or not.  But it seems likely we’ll need the full year’s data set before we start making much progress on this crucial issue (though surprises are possible, if the Higgs is sufficiently different from a Standard Model-type Higgs).  And indeed, even if the Higgs looks somewhat Standard-Model-Higgs-like by the end of the year, our knowledge will still be vague; through Phase 2 of the Higgs search, we’ll be continuing to address the issue for the rest of the decade, making more and more precise measurements of the properties of the Higgs, looking for any deviation from the Standard Model’s predictions.

All of this assumes the rumors are correct.  IF it is true that ATLAS and CMS see something of roughly the same size as last year, in exactly the same place in their plots, then that would mean that evidence for the existence of some type of Higgs particle in the 125 GeV/c2 range had firmed up considerably.  And that would be Very Big News.  Well — we’ll find out soon enough.

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON June 18, 2012

On Saturday I gave a lecture, newly minted, on how Einstein is perceived in the public eye, and on how the numerous misconceptions about Einstein affect the way many non-experts believe that science is actually carried out.  Doing the research for the lecture involved, among other things, going back to some original sources I’d never read or had only read a long time ago, looking a bit at Einstein’s notebook from the period around 1912 (online here), and re-reading large portions of a wonderful biography of Einstein that I’m afraid was written by a physicist for physicists — and consequently largely unreadable without technical background, but a must-read for anyone who has that background.  I refer here to Abram Pais’s famous biography: “Subtle is the Lord…”, whose title refers to Einstein’s famous quip: “Subtle is the Lord, but malicious He is not.”  (You can read about the origin of this quip in Pais’s book.)

I also enjoyed tracking down some videos online of various physical effects that Einstein explained, or that he predicted in advance.  These included videos (linked below) of (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON June 18, 2012

Reminder: New York, Saturday June 16th at 2pm, I’ll be giving a public lecture (click here for details): THE EINSTEIN OBSESSION: SCIENCE, MYTH AND PUBLIC PERCEPTION.

I’ve been doing a little work on my extra dimensions articles, adding one that describes how we know experimentally that the ordinary particles we’re made of (and most of the others we know about) can’t be moving in more than three spatial dimensions — more precisely, that any additional dimensions must be smaller in extent than 1/100th or so of the distance across a proton. The first half of the article is drafted; the second half, on what we know about dimensions in which no known particles can move but which are accessible to gravity and gravitons, will come soon, probably next week.  Comments and questions welcome as always.

Meanwhile, following up on Friday’s post about the End of the OPERA Not-Faster-Than-Light Neutrino Story: a paper has appeared by the LVD and OPERA experiments explaining how they worked together to confirm that OPERA’s two known problems (a fiber-optic cable connection and a clock running off-speed) did in fact cause their faulty measurement of neutrino speeds. This information was made public (in large part) back in March and I wrote about it in detail here.

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON June 13, 2012

Over the weekend, the Large Hadron Collider [LHC] passed a significant milestone: the amount of data collected so far in 2012 now exceeds the amount of data collected in 2011.  (The LHC is also running very efficiently right now.)  As you may recall, the data is being taken at a slightly higher energy than last year — 8 TeV instead of 7 TeV for each proton-proton collision — and among the benefits of this change are slightly higher probabilities of making Higgs particles.  In short, more Higgs particles (assuming they exist) have now been made this year than last, and if last year’s preliminary evidence of a Standard Model (or Standard-Model-like) Higgs particle [the simplest possible type of Higgs particle] with a mass of about 125 GeV/c2 turns out not to be a mirage, then the number of Higgs particles produced so far this year is about 100,000 for the CMS experiment and a similar number for the ATLAS experiment.  Most of these Higgs particles decay in ways that make them indistinguishable from other processes, but the dozens that decay to two photons and the handful that decay to two lepton/anti-lepton pairs will be the most important in this year’s search.

When will we see results from the new data on the search for the Higgs particle?  (Remember we’re still at the end of Phase 1 of this search, in which the goal is to find or exclude the Standard Model Higgs particle.) (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON June 11, 2012

In case you haven’t yet heard (check my previous post from this morning), neutrinos traveling 730 kilometers from the CERN laboratory to the Gran Sasso laboratory do arrive at the time Einstein’s special relativity predicts they would.

Of course (as the press mostly seems to forget) we knew that.  We knew it because

So the news from the Neutrino 2012 conference in Kyoto, on new data from May 2012 taken by OPERA and three nearby experiments, is no surprise to anyone who was paying attention back in March and early April; it’s exactly what we were expecting.

One thing that almost no one is reporting, as far as I can tell, is that CERN’s research director Sergio Bertolucci did not give the first talk on neutrino speeds in Kyoto.  That talk was given by Marcos Dracos, of OPERA.  Dracos presented both OPERA’s corrected 2011 results (with corrections based on the detailed investigation shown in March of the problems reported back in February) and also the new 2012 results, which were taken with a kind of short-pulse beams similar to that used in OPERA-2.  (A short pulse beam allows for a neutrino speed measurement to be made rather easily and quickly, at the expense of OPERA’s neutrino oscillation studies, which were the main purpose of building the OPERA experiment.)

Following Dracos’ talk, Bertolucci spoke next, and reported the results of the neighboring Borexino, LVD and ICARUS experiments on the May 2012 data, which along with OPERA are all bathed in the same CERN-to-Gran Sasso neutrino beam, and collected their data simultaneously.  All of the results are preliminary so the numbers below will change in detail.  But they are not going to change very much.  Here they are: neutrinos arrive at a time that differs from expectation by:

  • Borexino: δt = 2.7 ± 1.2 (stat) ± 3 (sys) ns
  • ICARUS: δt = 5.1 ± 1.1 (stat) ± 5.5 (sys) ns
  • LVD: δt = 2.9 ± 0.6 (stat) ± 3 (sys) ns
  • OPERA: δt = 1.6 ± 1.1 (stat) [+ 6.1, -3.7] (sys) ns

(Here “ns” means nanoseconds, and “stat” and “sys” mean statistical and systematic uncertainty.)  The original OPERA result was an early arrival of about 60 nanoseconds, about six standard deviations away from expectations.  You see that all the experiments are consistent with zero early/late arrival to about 1 standard deviation — almost too consistent, in fact, for four experiments.

So there is no longer any hint of any evidence whatsoever of a problem with the predictions of special relativity, and in particular with the existence of a universal speed limit.

A summing up is called for, but I want to write that carefully.  So unless something else comes up, that’s all for today.

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON June 8, 2012

Five out of five experiments agree: neutrinos do not travel faster than the speed limit.

Or more precisely: to within the uncertainties of current measurements, neutrino speed, for neutrinos with energies far larger than their masses, is experimentally indistinguishable from the speed of light in vacuum.  This is just as expected in standard Einsteinian special relativity, which would predict they move just below light speed, by an amount too small to measure with current experiments.

http://press.web.cern.ch/press/PressReleases/Releases2011/PR19.11E.html

Based on data taken in May 2012 using a beam of neutrinos sent from the CERN laboratory to the Gran Sasso lab, the four experiments ICARUS, LVD, Borexino and even OPERA (the source of  all the excitement) find results consistent with the speed of light, with uncertainties (at one-standard-deviation) about 10 times smaller than OPERA’s original measured deviation of neutrino speed from the speed of light.  The new results are consistent with ICARUS’s result from 2011 data.  Moreover, OPERA’s mistaken result from September and November 2011 — a claimed six standard deviations away from the expected speed — has now been corrected, following their detective work presented in March.  Even MINOS, a U.S. experiment, has revised their older result, which was previously slightly discrepant from the speed of light by a small amount (two standard deviations), and they find now that their data too are quite consistent with neutrinos traveling with light speed, though with much less precision in the measurement.

And so with a final quintet, sung in unison, this melodramatic comic OPERA buffa comes to a close.  As with all classic operatic comedies, there’s been crisis, chaos, and a good bit of hilarity, all the while with wise voices speaking reason to no avail, but in the end the overzealous are chastened, the righteous are made whole, everyone (even the miscreant) is happy, and all is well with the world.

Curtain!! Applause!!  Science Triumphant!!

Favorable review to follow when time permits.

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON June 8, 2012

A number of transitions to talk about:

First, I’m participating in a panel discussion today (Thursday June 7th) on the transition that has seen me add science writer and popularizer to my resume’. Here’s the link… free tickets required, click here for details and tickets. Sponsored by SoNYC (Science online New York City), panel discussion entitled “Reaching out of the Ivory Tower”, about the experiences of scientists who are reaching out to the public. Panelists: Ethan Perlstein, Sarah Weisberg, Matt Strassler, Jeanne Garbarino.  Location and time: Weiss 305, Rockefeller University, East 66th and York Ave. New York, NY, 7:00 PM.   Presenting science to the public in a digestible but honest form is something I feel is important, and I’ll have a few words to say about why I chose to do it now and why via a website and blog. And then I guess the floor will be open to questions, so come on by and ask one!

Reminder: again in New York, Saturday June 16th at 2pm, I’ll be giving a lecture (click here for details):  THE EINSTEIN OBSESSION: SCIENCE, MYTH AND PUBLIC PERCEPTION.

Next: I hope you all enjoyed seeing Venus in transit across the Sun Tuesday, in whatever method you chose. If you missed it live, there are of course opportunities to see films of the event — and they’ll save you time, since they’re all speeded up so that the hours pass in a minute or so. Nice views of Venus are complemented by several good-sized sunspots that are roughly the size of the Earth. Venus, you may recall, is the same size as the Earth, but as it was only a third as far away as the Sun yesterday, it appeared three times larger in radius (10 times larger in surface radius) than those sunspots. I managed to see it with the naked eye (with eclipse glasses), but just barely… so tiny! (By the way, if you missed my article on how a transit of Venus was used to obtain the first high-precision measurement of the distance to the sun, here’s the link.)

Here’s one of my own best shots, which I show you not because you can’t find better shots on the internet but because I have learned that most people do not realize you can get such nice views of the sun with so little work.

Venus in transit, at bottom.  Several sunspots dot the central region of the sun’s disk.  Photo of projection through binoculars onto white screen.  Image has been darkened slightly to sharpen contrast between sun and background.  Photo: M. Strassler 2012, all rights reserved.

It’s really quite easy.  And though there won’t be any more transits of Venus for us to see, there will be bigger sunspots, transits of Mercury, and solar eclipses to watch over the coming 15 years, so you may as well learn how to do this. You just aim the binoculars, big side toward the sun (as though someone were going to look at the sun — BUT DON’T LET ANYONE LOOK, of course), in the rough direction of the sun, wiggle the binoculars until the shadow of the binoculars becomes as small as it possibly can (which tells you they are aligned with the sun) and at that point the sun will shine through the two sides of the binoculars, giving you two images. Put a lens cover on one of the sides if you want to just get one image. Then let the image project onto something white and smooth that can serve as a screen. By moving the screen forward or back you can get a larger or smaller image; by using the focus on the binoculars you can bring the image of the sun into focus. Works great!

Here’s a picture, taken in a similar way, from the annular eclipse last month — a transit of the moon, even though we don’t usually call it that — taken the same way. I like this shot (though focus is imperfect and it was taken from a funny angle) because where the moon’s shadow touches the sun’s limb you can see a bit of light shining between mountain ranges on the moon!

A few seconds before annularity begins during the annular eclipse of the sun on May 20, 2012. Note, in the region where the moon’s silhouette touches the sun’s limb, a patch of sunlight shining through the mountain ranges on the moon. Light and dark regions at left and right of photo are due to shadows on the projection screen.  Photo: M. Strassler 2012, all rights reserved.

Venus, passing between the Sun and the Earth on Tuesday, has now transitioned from an object in the evening sky to one in the morning sky; if you want to see it, large and a very thin crescent through binoculars, you’ll need to get up early, before sunrise.  Not yet, though; it will be a few days before Venus is far enough from the Sun to pick out in the dawn sky.  For now, you can see Venus via the SOHO satellite, which blots out the sun so what’s nearby can be observed.

A final transition: Ray Bradbury died. Bradbury was one of the 20th century’s great science fiction writers, and I especially enjoyed reading his stories because he didn’t write classic geeky science fiction. His work was much more thoughtful and human than that. I think one could make a case that what made his writing unique was that he didn’t separate science from the rest of life.  It’s a good example for the rest of us to follow.

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON June 7, 2012

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