The Sun is Dying and Global Dimming – Brian Cox

Two mini-features from the CERN physicist, media star and scientific advisor to the movie Sunshine.

The Sun is Dying

The Sun will not live forever. It has enough fuel left, if our current understanding is correct, for another 5 billion years, at which point it will die. But could it be possible for the Sun to die much sooner, within the next 100 years even? From a scientific perspective, it should be said that this is very unlikely. But, it is also true that there is a lot about the universe that we do not understand.

Over the last few years astronomers have observed that there is extra “stuff” in the universe that we can see only by its gravitational influence on stars and galaxies. This stuff goes by the name of Dark Matter, and there is five times as much Dark Matter in the universe as there is normal matter, the stuff that makes up you, me, and the stars and planets we can see with our telescopes. What is this mysterious stuff? It’s possible, some scientists would say likely even, that this stuff is made of particles known as supersymmetric particles, a new and exotic form of matter that is high on the list of potential discoveries at CERN’s giant Large Hadron Collider, a 27km in circumference machine which begins operations this year after almost a decade of construction.

Theoretical physicists have spent many years calculating the properties of these supersymmetric particles, and we have a reasonable theoretical understanding of how they might behave. One possibility is that they could clump together into giant balls known as Q-balls. If this is true, then these heavy and exotic objects could have been made billionths of a second after our Universe began, and still be roaming the Universe today. It is speculated that, if a Q-ball drifts into the heart of a super-dense object such as a neutron star, it could begin to eat away at it’s core like a cancer, until the star is no longer massive enough to maintain itself and explodes in a violent explosion. Such explosions, known as gamma ray bursts, are seen in the Universe, although their cause is as yet unknown.

Could such a dangerous, exotic object drift into the Sun’s core and cause it to stop shining? It is likely that the Sun is many times too diffuse to stop a Q-ball – it would power right through. But maybe, just maybe, some strange exotic form of matter from the earliest times in the universe could settle deep within the Sun’s core, and disrupt its function enough to cause the catastrophic scenario seen in Sunshine. It’s far-fetched, but we have a saying in physics that anything that isn’t explicitly ruled out is therefore possible, so in the final analysis, you never quite know.

Global Dimming

It is now suspected that pollution in the Earth’s atmosphere, caused by industrialization and natural phenomena such as volcanic eruptions, may have significantly reduced that amount of sunlight reaching the Earth’s surface. It is estimated that this could have led to a cooling effect of over 1 degree overt he last 40 years, which would go some way to offsetting the effect of global warming. Global warming is caused primarily by increasing carbon dioxide levels in the atmosphere that prevent heat being radiated back out into space from the Earth’s surface.

The phenomenon of global dimming may therefore have saved us, so far, from the worst affects of climate change, although it has been noticed that as pollution levels have been reduced, particularly in Western Europe, the affects of global dimming seem to be reducing, leading to an accelerating temperature rise once again. We may therefore be in the paradoxical situation that reducing pollution might INCREASE the effects of global warming, leading us ever more quickly towards catastrophe.

This discovery isn’t all bad, however, because it may suggest a short term solution to climate change. Why not intentionally put pollutants, which may be designed to be benign in other respects, into the atmosphere to accelerate global dimming, and therefore slow the climate change caused by carbon dioxide emissions. Several suggestions along these lines have been made, including adding small particles to airplane fuel, and therefore using one of the main contributors to climate change, aircraft, to slow its effects. It’s an intriguing possibility, and one that is the focus of significant research, although it should be said that we cannot at present predict the effects of such fine-tuning of the climate, so global dimming shouldn’t be seen as a means to allow us to continue to increase carbon dioxide emissions.

Brian Cox is science advisor to the movie Sunshine – see www.sunshinemovie.co.uk

The Quantum Universe: everything that can happen does happen – Brian Cox & Jeff Forshaw ****

Brian Cox has picked up a lot of fans (and a few parodies) for his light and fluffy ‘here’s me standing on top of a mountain looking at the stars’ TV science shows – no doubt a fair number of them will rush out and buy his latest collaboration with Jeff Forshaw. They will be disappointed. So, I suspect, will a number of My Little Pony fans, as with its rainbow cover and glittery lettering it only needs a pink pony tail bookmark to complete the look.

The reason The Quantum Universe will disappoint is not because it is a bad book. It’s brilliant. But it is to Cox’s TV show what the Texas Chainsaw Massacre is to Toy Story. It’s a different beast altogether.

As they did with their E=mc2 book, but even more so here, Cox and Forshaw take no prisoners and are prepared to delve deep into really hard-to-grasp aspects of quantum physics. This is the kind of gritty popular science writing that makes A Brief History of Time look like easy-peasy bedtime reading – so it really isn’t going to be for everyone, but for those who can keep going through a lot of hard mental work the rewards are great too.

More than anything, I wish this book had been available when I started my undergraduate course in physics. It would have been a superb primer to get the mind into the right way of thinking to deal with quantum physics. Using Feynman’s least action/sum over paths with ‘clocks’ representing phase, the authors take us into the basics of quantum physics, effectively deriving Heisenberg’s uncertainty principle from basic logic – wonderful.

They go on to describe electron orbitals, the mechanics of electronic devices, quantum electrodynamics, virtual particles in a vacuum and more with the same mix of heavy technical arguments, a little maths (though nowhere near as much as a physics textbook) and a lot of Feynman-style diagrams and logic.

The reason I think I would have benefited so much is that this book explains much more than an (certainly my) undergraduate course does. Not explaining why quantum physics does what it does – no one can do that. But explaining the powerful logic behind the science, laying the groundwork for the undergraduate to then be able to do the fancy maths and fling Hamiltonians around and such. It is very powerful in this respect and I would urge anyone about to start a physics degree (or in the early stages of one) to read it. I would also recommend it for someone who is just really interested in physics and is prepared to put a lot of work into reading it, probably revisiting some pages several times to get what Cox and Forshaw have in mind – because they don’t ease up very often.

What I can’t do, though, is recommend this as general popular science. It isn’t the kind of excellent introduction that gives you an understanding of what’s going on in quantum theory, a view of the mysteries and a broad understanding of what the topic is about. This book is just too hard core. I’d suggest that 90% plus of popular science readers shouldn’t touch it with the proverbial barge pole. If that sounds condescending, it isn’t meant to be. Good popular science can and does have a lot more content and thought provoking meat than a typical Brian Cox TV show – but this book goes so much further still than that, inevitably limiting its audience.

Hardback:  

Also paperback from June 2012: 

Also on Kindle:  

Also on Audio CD:  

Review by Brian Clegg

Why Does E=mc2? – Brian Cox & Jeff Forshaw ****

Brian Cox is a dream for any publisher (sorry, Jeff Forshaw, but we haven’t heard of you). The media’s darling physicist at the moment, Cox is sometimes described as the popstar physicist, partly because he looks like one, but even more remarkably, because he was one. Although now Professor of Particle Physics at Manchester University (though confusingly, according to the bumf, he lives in London – that’s quite a commute), he was once part of the band D:Ream. He’s also a nice guy – I’ve done couple of gigs with him (speaking engagements, not music), and though a little over-enthusiastic about the movie world at the time, he was very friendly.

You might expect, with Cox on board, that this would follow the approach of TV science – lots of ‘gee, wow, amazing!’ but light on nuts and bolts science. But not a bit of it. In fact, if Cox and Forshaw had taken the same advice about equations as Stephen Hawking, the chances are they would have expected to have around 2 readers.

This is primarily a book about the origins of the world’s most famous equation, but rather than just give fun background, some special relativity and some handwaving, this pair plunge in and really do explain how E=mc2 is derived, something that isn’t generally done in popular science because, frankly, it’s pretty hard going. They don’t stop there either. They go into the master equation of the standard model of particle physics, explaining how it is derived from gauge symmetry, exploring the different components of the equation and giving by far the best explanation of the Higgs field/Higgs boson that I have ever seen. In this, the book is absolutely masterful.

What I was a little disappointed with, having heard Cox’s eloquent speaking, is the rather stiff writing style. Although it tries to be friendly, I felt a bit like I was… well, being talked to by a couple of professors. There’s a lovely example of this where they quote Kurt Mendelssohn’s book on Lavoisier’s widow where she is said to have led Count Rumford “a hell of a life.” Cox and Forshaw then comment: ‘the book was written in 1966, hence the quaint turn of phrase.’) You can almost see the pursed professorial lips.

I loved this book, which perhaps makes it rather surprising that I only gave it four stars. If you’ve at least a physics A level and are about to set out on a physics degree (or, like me, you’ve got a rusty physics degree), it’s phrased at just the right level. But I felt it would be hard going for a general reader without that background. I had to re-read several bits to be sure what the writers intended, and in the end there’s a reason most popular science books don’t have this level of technical detail.

So, not quite the perfect popular science book, yet certainly one of 2009′s gems.

Paperback:  

Also on Kindle:  

Review by Brian Clegg