Category Archives: Physics

IOP Newton Lecture, 'From Mars to the Multiverse', 28 February

From Mars to the Multiverse

Prof Martin Rees, Lord Rees of Ludlow

Institute of Astronomy

Date: Thursday 28 February 2013

Venue: Institute of Physics, 76 Portland Place, London, W1B 1NT

Time: 17.30 (registration from 17.00)

rees
Prof Martin Rees

‘Astronomers have made astonishing progress in probing our cosmic environment. We can trace cosmic history from some mysterious “beginning” nearly 14 billion years ago, and understand in outline the emergence of atoms, galaxies, stars and planets.

But the key parameters of our expanding universe — the expansion rate, the geometry and the content — were established far earlier still, when the physics is still conjectural but can be pinned down by future observations. These advances pose new questions: What does the long-range future hold? Should we be surprised that the physical laws permitted the emergence of complexity? And is physical reality even more extensive than the domain that our telescopes can probe? This illustrated lecture will attempt to address such issues.’

Follow the link below to register.

Link
The Newton Lecture

Note
The original message is from Claire Copeland, Science Support Officer at the Institute of Physics.

Prof. Peter Higgs been recognised in the New Year Honours

Prof. Higgs, whom the Higgs boson is named after, is now a member of the Order of Champions of Honour. The honour has no title, but consists of the Sovereign, plus no more than 65 Companions of Honour.

Higgs Prof. Higgs

Other Companions of Honour include Prof. Stephen Hawking and Sir David Attenboroug.

The Higgs Boson
Prof. Higgs developed the idea of electroweak symmetry breaking to explain the masses of the Z and W bosons [1]. The Higgs-Kibble mechanism gives rise to the mass of all the massive elementary particles and predicted the existence of a new particle given the title “the Higgs boson”.

higgs simulationComputer simulation of particle traces from an LHC collision in which a Higgs Boson is produced. © CERN. Image credit: Lucas Taylor

Only recently at the LHC has there been evidence that the Higgs boson is realised in nature. CERN announced on 4 July 2012 that they had experimentally established the existence of a Higgs-like boson and that further study is needed to established if this really is a standard model Higgs boson, [2,3].

The Nobel prize?

Is a Nobel prize in Physics the next big award for Prof. Higgs? We will have to wait and see.

References

[1] Peter Higgs, Broken Symmetries and the Masses of Gauge Bosons, Physical Review Letters 13 (16): (1964) 508–509.

[2] The ATLAS Collaboration, Observation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC, Phys.Lett. B716 (2012) 1-29. (arXiv:1207.7214 [hep-ex])

[3] The CMS Collaboration, Observation of a new boson at a mass of 125 GeV with the CMS experiment at the LHC, Phys.Lett B716 (2012) 30–61. (arXiv:1207.7235 [hep-ex])

Links
The Order of Champions of Honour

Prof. Higgs Website at the University of Edinburgh

Government boost to graphene research

The Chancellor, George Osborne, has announced a £21.5m investment fund to boost the development of the new wonder material graphene.

The £21.5m investment fund would aim to take the technology from the lab to the factory floor.

George Osborne

Graphene
Graphene is a material made carbon atoms arranged in a regular hexagonal pattern, similar to graphite, but in a one-atom thick sheet. Graphene has many unusual electrical and mechanical properties that make it interesting from a fundamental science point or view, but also lend this wonder material to applications.

graphene
Image courtesy of AlexanderAlUS

Andre Geim and Konstantin Novoselov, both based at the University of Manchester won the 2010 Nobel Prize in Physics for demonstrating some of the properties of graphene.

Geim
Andre Geim

Funding
EPSRC identified the most promising graphene-related research projects in British universities that would benefit from state funding.

For example, Cambridge will receive more than £12m for research into graphene flexible electronics and opto-electronics. Other UK universities, including Manchester will also receive money.

We need to support our universities, they’re one of the jewels in the crown of the British economy

George Osborne

Link
BBC News

Snakes Physicists on a plane

on a plane

Physicists from Japan have grown crystals in near zero gravity by using a diving airplane [1]. The idea was to examine crystal growth under such conditions to uncover phenomena usually masked by gravity’s effects.

[youtube:https://www.youtube.com/watch?v=xkjzKjGo40A&feature=player_embedded]

For more details follow the link below or the original paper cited.

This man had nothing to do with it…

Samuel L. Jackson

Link
IOP News Physics on a plane: crystals made under zero gravity

Reference
[1] Takuya Takahashi, Haruka Ohuchi, Ryuji Nomura and Yuichi Okuda, Ripening of splashed 4He crystals by acoustic waves with and without gravity, 2012 New J. Phys. 14 123023 (link)

Physics World's favourite images of 2012

Physics World (IOP’s magazine) have collated 12 images that demonstrate the visual beauty that can be found in physics.

My personal favorite is this the Weaire–Phelan foam, which I reproduce below.

foam

The Weaire–Phelan foam is believed to be the lowest energy structure for a foam formed of equal-volume bubbles. The foam was created using a special template in a solution of water and Fairy Liquid, with bubbles being introduced by releasing nitrogen gas from a glass capillary. The resulting foam was photographed using a digital SLR camera.

Link
Our favourite pictures of 2012 (Physics World)

IOP Special Report on India

As we are all aware India has one of the fastest growing and largest economies in the world. The economy of India is the tenth-largest in the world by nominal GDP and the third largest by purchasing power parity (PPP) (see here).

Indian scientists are not short of money. They have a space program (Indian Space Research Organisation) as well as a nuclear arsenal.

On that note, Great Britain will be phasing out financial aid to India by 2015, instead focusing on technical assistance (BBC News). To me personally, that makes sense and will be of benefit to both Indian and British scientists.

The IOP Report
The Institute of Physics (IOP) have written a report on India.

For today’s leading physicists in India, money for research is thankfully not in short supply. But as this Physics World special report makes clear, what India currently lacks is a critical concentration of highly capable scientists who can really make the country a world leader in research and boost the nation’s innovation. This special report shows, however, that India is starting to tap the country’s true potential through a series of bold educational initiatives and novel research facilities. I hope you find this report stimulating and please do e-mail your comments to pwld@iop.org.

Matin Durrani, Editor of Physics World

Link

report

Special Report India

Physics World’s special report discovers that India is starting to tap the country’s true potential through a series of bold educational initiatives and novel research facilities.

Stephen Hawking wins special physics prize

Special Fundamental Physics Prizes have been awarded to a team of seven scientists who led the efforts at CERN’s Large Hadron Collider (LHC) and, separately, to Stephen Hawking for his discovery that black holes radiate.

Hawking

These two awards highlight how strong a role British physicists play on the world stage. From the three British-based physicists leading efforts at LHC – Lyn Evans, Michel Della Negra and Tejinder Singh Virdee – to Stephen Hawking, we should rightly cherish our nation’s strength in physics.

Professor Sir Peter Knight, President of the Institute of Physics.

Black holes are not black!
In 1975 Hawking published a paper with a rather surprising result: if one takes into account quantum theory black holes are not quite black. Rather, a black hole glows slightly due to “Hawking radiation”, which consists largely of photons and to a lesser extent other particles.

The corresponding temperature is

\(T \approx \frac{1.227 \times 10^{23} }{M}\) Kelvin, and here the mass is in KG.

Because of this, the temperature would only be significant for very light black holes. For example, a 30 solar mass black hole has a temperature of about \(2\times 10^{{-}9}\) Kelvin and the corresponding luminosity is about \(10^{{-}31}\) Watts. Bigger black holes would hardly radiate at all. This would be completely swamped by other sources of radiation including the CMBR.

Evaporation of a micro black hole
Black holes get the energy for the Hawking radiation from their rest mass. So, assuming nothing is falling into the black hole, a radiating black hole will be loosing mass. For astrophysical black holes this loss will be miniscule. The evaporation time for a black hole of 30 solar masses is about \(10^{60}\) times the age of the Universe!

For much much smaller black holes Hawking radiation could lead to compete evaporation. For example, a black hole with the mass of about a mountain could evaporate in a time scale that is less than the age of the Universe.

However, no-one is really sure what happens to a black hole near the end of its evaporation.

The black hole information paradox
Classically, there are only three things we can know about a black hole; its mass, its angular momentum and its electric charge. These are the only parameters that describe a classical black hole. I paraphrase this as “black holes do not care what they eat”.

No matter what properties the matter that falls into a black hole has, say baryon number or lepton number, the black hole classically only cares about the mass, angular momentum and electric charge. All the other information is hidden inside the black hole away from the rest of the Universe.

So now suppose our black hole evaporates and disappears. An important property of Hawking radiation is that it is thermal: that is completely random. The information content of a black hole (what it has eaten!) appears to be lost when it dissipates.

What happens to this information is a far from understood question in physics.

Hawking’s work on black hole radiation has posed more questions about nature than it has really answered. That is the true sign of great work.

Links
Fundamental Physics Prize Foundation News

IOP News

An interview with Dr Helen Czerski

Dr Helen Czerski, Physicist and oceanographer, is a well-known BBC science presenter. Her work includes the major BBC2 series ‘Orbit: Earth’s Extraordinary Journey’, broadcast in March 2012. Recently she filmed Operation Iceburg for BBC2 and is a contributor to Dara O’Briain’s Science Club.

Helen

She agreed to answer a few questions I had…

Science and Popularisation

What first got you involved in science, and in particular physics?

I don’t really feel that I ever “got involved” – it was just something I did and was interested in. I’m lucky that my parents encouraged us to experiment with the world in a non-pushy way – if I said “what happens when you do that?”, they’d just say “well, let’s try it and see”. I must have shown some specific interest in physics early on because my mum bought me a copy of “A brief history of time” when I was 10 or 11. But I was interested in all sorts of things, like dinosaurs and making stuff from clay, building treehouses, environmental issues, baking and languages. My parents just encouraged us in whatever we were interested in, and the strongest and most important message I ever got from them was “do your best”. That’s crucial – they weren’t bothered about whether we succeeded or not, but they valued trying things out. And they wanted us to be happy far more than they wanted “success”.

As time went on, I think that I chose to read a lot of popular physics books, and I knew from fairly early on that my interested tended towards the sciences. But I very consciously took every opportunity to study other things, because I felt that I’d do enough science later on.

How did you get involved in the popularisation of science? 

Well, going right back, I remember giving a talk on atomic physics to the local women’s group (which my mother was part of) when I was 17. So I suppose that counts as the first time I did anything like that. My Dad has always said that I’m a natural teacher, and when I was younger that mostly came out in the sports coaching that I did. During my PhD, I got involved in doing demonstrations during National Science and Engineering Week, and that led to other public lectures and talks. I was always happy to share my enthusiasm for science, and if that meant fun demos, so much the better!

Which medium  do you think is the most effective at popularising science?

There is no one medium, because what you say is not anywhere near as important as what your audience hears. If you say something in a format that your audience doesn’t see, it’s pointless. So the most effective medium is whatever your audience finds most convenient, and that’s different for every individual. Obviously, tv has a huge reach, but the ways that people get information are changing over time. I think that the one thing that will always be popular is seeing an enthusiastic and charismatic individual in person, and being brought into the world of the human being who is standing right in front of you. In an ideal world, we wouldn’t have “science popularization” because everyone who works or uses science and technology would naturally share their knowledge of it with the people around them, and that would be the most effective way of encouraging enthusiasm for science.

What, in your opinion, should be the ultimate goal of science popularisation?

To dispense with the need for conscious science popularization. It’s not a phrase I like. I think that we need science to be part of our culture just like music, literature, art, politics and economics, and we can all have some level of natural curiosity about it. I would love everyone to appreciate science as an important and fascinating part of their world, and to be able to find out as much about it as they liked. In an ideal world, it would be valued appropriately, and it wouldn’t be necessary to “popularize” it.

What were the challenges for you  during the filming of Operation Iceberg?

Being in between two worlds. Usually, in that environment, I’m there either because I’m doing my own experiment or I’m there because I’m filming a tv programme. This time, I was halfway – slightly more on the tv side of things, and without an experiment that I was responsible for by myself. I found that very odd – it was like being the only person in the room who spoke two languages when everyone else only spoke one or the other.

We really enjoyed science club, did you enjoy making it?

The studio days for science club have been some of my favourite days this year. It really is like an inclusive club of fun people, and everyone has something interesting to contribute.

Are we going to see a lot more of you on the BBC?

I’m working on a couple of other programmes at the moment. The one I’m spending most of my time on at the moment is a BBC4 programme all about bubbles.

Research

Can you say a few words about your research?

I study the bubbles underneath breaking waves, and how they break apart and join together in different conditions. This is important because these bubbles act as a transport mechanism between the atmosphere and the ocean, and we need to understand the small-scale mechanisms contributing to global-sized transport effects. I like it because it’s physics that happens on a scale that you can see. My lab experiment is the size of a bench, and you can really see what’s happening. I’m much more interested in phenomena that I can see directly, rather than quantum mechanical things that I can’t experience directly, or cosmological things that are far too far away ever to touch. What gets me going is “the physics in the middle”.

Which one of your papers are you most proud of, and why?

I was the first person to measure the thickness of the coating surrounding an ocean bubble in situ. All ocean bubbles are coated with a thin layer of organic material (effectively natural bubble bath), and it controls a lot of their behaviour but it’s hard to measure. You can’t take the bubble out of the water to look at it directly. I used a combination of acoustical and optical techniques to estimate the coating thickness while the bubble was still in the ocean, from a data I collected in the Pacific. I like it because it was a novel use of experimental data, and I hadn’t thought that I could make that measurement before I collected the data. It was a minor eureka moment when I realized that I could.

What are the major questions faced today in you area of research?

The biggest question is how to integrate all the many effects that work together to influence how our planet works. There are too many for any one person to be able to hold them in their head. How do we manage the data so that we can still get insights into what it means? How do we integrate all the biological, chemical, physical and geological data to test our models accurately? When data sets are too big for a human to hold them in their mind, we lose the human’s amazing ability to recognize patterns. How do we compensate for that?

Anything else?

I think that the world around us is full of physical toys – everyday things that we are completely used to, but which are each an amazing demonstration of some scientific principle. You don’t need to go to far away places or use special microscopes to see fascinating things. They’re all around you. The world would be a richer place if everyone got a bit better at looking at everyday phenomena and asking a few more questions than normal.

About Helen

Helen

Helen is a Physicist, oceanographer and broadcaster with a passion for science, sport, books, creativity, hot chocolate and investigating the interesting things in life. She currently works at the Institute for Sound and Vibration Research in Southampton, and is a science presenter for the BBC.

You can find out lots more about Helen via her website.

Paul Frampton sentenced for drug smuggling

Paul Frampton, a physicist from the University of North Carolina, was sentenced to four years and eight months in prison after being found guilty of drug-smuggling on November the 21st.

frampton

Paul Frampton

Frampton (68) got into trouble, rather naively, after flying from North Carolina to Bolivia, where he was planning to meet a 32-year-old Czech-born lingerie model Denise Milani. He believed he had been chatting with her on the internet.

denise-milani

Denise Milani, image courtesy of FHM

She did not show up, instead he was met by a man. This man then asked him to take “Milani’s” suitcase to Buenos Aires, where she would then meet up with him. There is no evidence that Milani knew her persona was being used in this way.

Frampton then tried to board a plane back to the US at which point he arrested after airport-security officials discovered the cocaine inside a false lining of the suitcase.

Frampton has always claimed that he was innocent of the drug-smuggling charges. He insists that the cocaine was placed into the luggage without his knowledge.

Despite health issues while locked up, Frampton continued to supervise his two current PhD students by phone and managed to place preprints on arXi.

Link

IOP News

Help Paul Frampton

FHM Magazine

Supersymmetry remains elusive

Results from the Large Hadron Collider (LHC) at CERN point show that the rare B-meson to a muon and antimuon decays are consistent with the standard model. It was hoped that the details of these rare events would provide evidence of supersymmetry, at least for energies up to 8 TeV.

Researchers working on the LHCb experiment announced their results on Monday at the Hadron Collider Conference in Kyoto. A preprint is available on the arXiv.

However, this is not actually inconsistent with supersymmetry, the measurements are still compatible with some supersymmetric theories. For example, Prof. Gordon Kane argues that models based on superstring compactifications are quite compatible with the LHCb results. You can read more about this here.

The energy of the collisions at the LHC will be increased from the current 8 TeV to 14 TeV, which will be engineered over the 2013–2014 shutdown. It is possible that signals of supersymmetry may be found at this higher energy.

Right now it seems that the standard model has again passed at the tests, which include he discovery of the Higgs and the details of the rare B-meson decays.