We decide to build a wall.

Add some signage designed by Daniel Clark and we are ready for our first Open Lab. at Guest Projects.

1704 Laboratory Open.jpg

The idea is that we work in the space and are open for visitors to drop in and see what we are up to and chat about the work and the ideas around dark matter research that we are investigating.

We set up a reading table and information hub with artist profiles, research material and info on Boulby Underground Laboratory   which we visited last spring to discover for ourselves this hidden world where dark matter research and experiments take place.

During the first two weeks at Guest Projects we ran workshops and tested ideas in the space.

Chroma-key body suits needed a test run from Amy Gear.

1704 Amy greensuit

Elizabeth Murton was considering dark matter as a connective material in the universe, setting up a tension of competing forces that may be as powerful as those of fission and fusion.

1704 Elizabeth Murton testing

I ran Cloud Chamber workshops.

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Thankfully everyone was able to ‘capture’ their own particle trails in the mini cloud chambers they made and were duly captivated by the tiny missiles they observed.

1704 Cosmic Trail 6

The cloud chamber gives us a glimpse into the invisible world of particles produced in the radioactive decay of naturally occurring elements and those generated when cosmic rays strike the top of the Earth’s atmosphere.

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It is a sealed environment containing a supersaturated vapour of pure alcohol, warmed at the top and super cooled at the bottom with dry ice.

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Charged particles passing through the chamber cause the alcohol molecules to gain an electric polarisation and condense into liquid droplets which look like tiny airplane trails.

1704 Cosmic Trail 9

To see the trails the particles leave as they tear through the cloud it must be very dark with a bright light shining across the floor of the chamber.

1704 Cloud Chamber setup

The activity takes place very near to the base of the chamber just a centimetre or two deep.

1704 Cosmic Trail 5

There is so much activity going on and these particles are whizzing through us all the time.

1704 Cosmic Trail 4

It seems we shouldn’t actually see some of these visitors at all but due to the weird way special relativity works we do. Muons are typically produced around 15 km up in the atmosphere, a distance which takes around 50 microseconds to cross at the speed of light— this is over 20 muon lifetimes and so they shouldn’t be able to make it to the earth’s surface before they decay.

1704 Cosmic Trail 1

However, since they are travelling quite near the speed of light, time in their frame of reference is significantly dilated as seen by an observer on Earth, meaning that a significant fraction can, in fact, make it to the surface. I have to be honest I can’t get my head round this but I love the idea of a particle having its own time frame of reference.

1704 Cosmic Trail 3

As well as Muons we see particles from background radiation. Radioactivity is a random naturally occurring process.  Alpha particles are released by high mass, proton rich unstable nuclei. The alpha particle is a helium nucleus; it consists of two protons and two neutrons. It contains no electrons to balance the two positively charged protons. Alpha particles are positively charged particles moving at high speeds. Beta particles are emitted by neutron rich unstable nuclei. Beta particles are high energy electrons. These electrons are not electrons from the electron shells around the nucleus, but are generated when a neutron in the nucleus splits to form a proton and an accompanying electron. Beta particles are negatively charged. For the particle to cause a trail it must have a charge which will ionize the vapour as they pass through, we don’t see neutrinos as they do not have a charge.

1704 Cosmic Trail 2Once you have the right set up it’s surprisingly easy to witness this turbulent landscape with it’s own little microclimate.

1704 frosty edges

Melanie King ran a day of hypnotic workshops painting with phosphorescent powder and using lasers to activate the phosphorescence which absorbs light then slowly releases it, allowing patterns to build up, layer and fade away.

1704 Melanie King phosphorence workshop 1

1704 melanie king Phosphoresence

The very knowledgeable Jennifer Crouch founder of Making in Transit and member of Art/Physics collective Jiggling Atoms ran a Super Symmetry workshop for us transforming the space with shimmering two way reflective veils

1704 Jennifer Crouch Super Symmetry 1

explaining the different types of particle and how easy or not it is to detect them, the contested theories of supersymmetry and the use of a black mirror (Claude glass) for observing nature

new particles were ‘created’, observed and drawn

Amy Gear invited anyone who identified as female to join a green screen/self defence workshop under the guidance of martial arts expert Jiff Higman to explore the visibility of women in the universe. The points of body contact echoing the anticipated nudge of the target xenon nucleus when a dark matter particle hits it and causes a scintillation of energy that the scientists can record. In the final video work only 5% of the bodies will be visible.

There was a spellbinding Hour Of Listening curated by Jennifer Boyd and Amy Pettifer. As the light faded we listened to Dark Matter Gushes From The Mouth Into The Open Air – ‘Latent gurgles, murmurs rising… a tone begins in the depths of the belly and strives in the throat before escaping – a burst of vocal dark matter. ‘

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Jocelyn Monroe, Professor of Physics at the Royal Holloway University of London kindly shared some links to her research areas.

1704 SNO chamber

She works in an underground laboratory SNOLAB where the DEAP dark matter search experiment takes place in Canada. She also works with the The Dark Matter Time Projection Chamber project and has written an article for symmetry magazine about the search for the dark matter wind which could give an idea of the direction dark matter comes from.

Lecturer in accelerator physics at Lancaster University and a member of the Cockcroft Institute of Accelerator Science and Technology, Ian Bailey shared his fascinating research searching for new particles and forces at both high energies and low energies.

1704 Ian Bailey cascade

He works with microwave cavities that are in some ways similar to household microwave ovens to look for the effects of hypothetical particles such as axions or hidden-sector photons. These particles are sometimes generically called weakly-interacting slim particles (WISPs). Just like their heavy cousins, the WIMPs (weakly interacting massive particles), WISPs may also be a major constituent of dark matter.

1704 Ian Bailey Cascade cooling

If they exist, hidden-sector photons (dark photons) would allow normal light to penetrate through walls in a way that it cannot normally do. The experiments that look for this effect are called light-shining-through-a-wall experiments and one such experiment has taken place at the Cockcroft Institute recently. It may be possible that dark matter could have subtle effects on the motion of light.

So from looking into this a bit it seems regular photons are changed to dark photons (axions)  by applying an intense magnetic field or maybe some other force – a barrier is set up that regular photons cannot pass through but dark photons can – the dark photons pass through the barrier and then turn back into visible photons which can be detected.

He is also involved in the design of the International Linear Collider, a potential new 31 km long particle accelerator which will try to produce WIMPS by colliding intense beams of electrons and positrons (anti-electrons) at high energies.

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I was invited to write a lead article for Run Riot listing site of cultural happenings in and around London explaining how the project had come about. Great dealing with the lovely Ava Szajna-Hopgood.

Elizabeth Murton curated and expertly chaired our Lab. Talks+ sessions. We opened with a live link to Boulby Underground Laboratory for a remote tour with lab. director Prof Sean Paling who made our visit to the lab. last year possible.

1704 live link to Boulby

Chair of UK Dark Matter, LUX collaborator, UCL lecturer and enormously generous supporter of our project Dr Cham Ghag gave us an in depth talk on the latest dark matter detection experiments and theories

1704 Guest Projects symposium Cham Ghag

Extraordinarily super clever Libby Heaney had us entangled with quantum theory, weaving and whispering and negotiating being in two states at the same time.

UCL History and Philosophy of Science lecturer Dr Chiara Ambrosio gave us her insights on visualising the invisible, and what can happen when art and science collide

1704 Guest Projects symposium Chiara Ambrosio

ending with a panel discussion joined by Kate Fahey on ideas from the day

1704 Panel discussion

and lots of conversations over supper…

I had finished etching the pentagon plates and I had made the dodecahedron frame – it was time to put it all together.

1704 test plates on frame

I did a test fit. Then spent 5 hours back at home heat pressing the plates with sublimation images; hints of dream worlds.

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I was quite pleased with the results and went to bed

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In the morning the colours had undergone some reaction to the metal and had either vanished or changed to a sort of purple hue (funnily enough often used to colour dark matter visualisations). I was also feeling I might just be making a large Moroccan lamp.

Time to embrace unexpected outcomes….

 

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