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Nuclear Physics B Proceedings Supplement 00 (2014) 1–6

Nuclear Physics B Proceedings Supplement

The Sciences ACO Light and Matter Museum

Nicolas Arnauda,b,∗, Martine Bessona,b, Henri Borieb, Paul Brunetb, Maurice Chapellierb,c, Andr´e Damanyb, Elisabeth Dartygeb, Nicolas Deleruea,b, Pierre Dhezb, Yves Ducrosb, Marie-Pauline Gacoinb,d,e, Jacques Haissinskia,b, Bernard Jean-Mariea,b, Jack Jeanjeanb, Roland Jolivotb, Serge Julliana,b, Guyve Khalilib,f,

Jean-Michel Ortegab, Robert Riskallab, Patrick Roudeaua,b, Michel Sommerb, Christophe Sottyb,c,1, Georges Szklarza,b

aLAL, Univ Paris-Sud, CNRS/IN2P3, Orsay, France

bThe Sciences ACO association, France

cCSNSM, Univ Paris-Sud, CNRS/IN2P3, Orsay, France

dFondation de Coop´eration Scientifique du campus Paris-Saclay, France

eSynchrotron SOLEIL, L’Orme des Merisiers - Saint-Aubin - BP 48 - 91192 Gif sur Yvette Cedex, France

fLaboratoire Aim´e Cotton, CNRS/Univ. Paris-Sud/ENS-Cachan

Abstract

Sciences ACO is a non-profit association based in Orsay (France). It manages a Museum of Light and Matter visited by more than 1,000 people each year. In this unique place, scientists and cultural mediators preserve, exhibit and comment on items of the history of science & technology, to pass on the knowledge of this heritage to the audience. Sciences ACO visitors – among them many high school students and teachers – come to learn about the progress of science and the technology evolution over more than four decades. Sciences ACO is more than just a historical museum: it is a driving force for the development for outreach and pedagogical activities on the Paris-Sud University campus and in the neighboring towns. The history, the present activity and the prospects of the Sciences ACO association are presented in this article.

Keywords:

Accelerator, Collider, Education, Museum, Outreach, Storage Ring, Synchrotron light

1. Origin and history of the Sciences ACO associa-

1

tion

2

1.1. The LAL-LURE accelerator complex

3

The Sciences ACO museum [1] is located at the cen-

4

tre of the LAL-LURE accelerator complex [2], which

5

was awarded the Historic Site label by the European

6

Physical Society in September 2013 [3]. This site dates

7

back to 1956 when the ”Laboratoire de l’Acc´el´erateur

8

Lin´eaire” (LAL, today a joint unit of the CNRS/IN2P3

9

Corresponding author

Email address:[email protected](Nicolas Arnaud)

1Now at KU Leuven in the Nuclear Spectroscopy Group.

and of the Paris-Sud University) [4] was set up in Or-

10

say to build and operate a state-of-the-art linear accel-

11

erator (linac). It was operated from 1959 to 2003, pro-

12

viding high intensity electron and positron beams of en-

13

ergy up to 2.3 GeV. In the meantime, many upgrades

14

were performed to improve its performance and major

15

facilities added, ranging from electron-positron collid-

16

ers to synchrotron light sources. In the early 1970’s the

17

”Laboratoire pour l’Utilisation du Rayonnement Elec-

18

tromagn´etique” (LURE) was created in close technical

19

connection to LAL to develop a wide research program

20

based on synchrotron light: materials science, chem-

21

istry or structural biology. Nowadays, the LURE has

22

become SOLEIL [5], the French third generation syn-

23

chrotron source (located nearby) while the LAL is still

24

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Figure 1: Access map for the Sciences ACO museum.

a major laboratory whose research activities range from

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participation in the LHC experiments to contributions to

26

the Planck satellite observations.

27

1.2. The ACO collider

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The ”Anneau de Collisions d’Orsay” (ACO) stored

29

its first beam in 1965, two years after the observation

30

at LAL of the first ever electron-positron collisions with

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the AdA collider [6]. Designed and built in Frascati un-

32

der the leadership of Bruno Touschek, AdA was brought

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to Orsay in 1962 to benefit from the linac high particle

34

injection rates. This pioneering work opened an entirely

35

new field in accelerator science – in particular, the so-

36

called Touschek effect was discovered and understood

37

while AdA was running at LAL.

38

ACO, whose operation ended in 1988, was first used

39

as a 1100 MeV electron-positron collider. It lead to im-

40

portant discoveries in accelerator physics and to many

41

pioneering measurements of vector meson properties.

42

In 1973, ACO became the first storage ring in Europe

43

available to synchrotron light users. Ten years later, a

44

free-electron laser was successfully operated at ACO –

45

the second in the world, it was the first one in the visible

46

bandwidth and the first at a storage ring.

47

Rather than being decommissioned and disassembled

48

like almost all accelerators in the world once they are

49

turned off, ACO was carefully preserved by the very

50

people who worked on it. In 2001, the machine was

51

recognized as a French heritage monument.

52

Figure 2: Aerial view of the LAL in 1981.

1.3. The Sciences ACO Light and Matter Museum

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As early as 1993, the ”Sciences ACO” association

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was created by physicists and engineers who worked on

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the storage ring. Recognized as a general interest asso-

56

ciation in France in 2011, it is still very active and is now

57

bringing three generations of scientists together. The as-

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sociation program is twofold: to circulate the rich ACO

59

history (in particle accelerator, collider and synchrotron

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light physics) and, based on it, to shed light on today’s

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science.

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Sciences ACO operates a ”Light and Matter Mu-

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seum” – see access map in Fig. 1 – open on request

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and during special events: European heritage days, na-

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/Nuclear Physics B Proceedings Supplement 00 (2014) 1–6 3

tional science festival, etc. It welcomed about 1,600 vis-

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itors in 2013 – roughly 50% students and teachers, and

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50% general public. Joint visits with the historical Sci-

68

ences ACO partners LAL and SOLEIL are often orga-

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nized, since seeing real scientific and technological in-

70

struments renews the visitors’ attention and makes out-

71

reach conferences more concrete. In addition, Sciences

72

ACO is also hosting and organizing various events, in

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particular on the theme of art & science. This not only

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widens the museum audience, but it also helps in getting

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more support from local authorities. This complements

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the Sciences ACO primary mission which is to promote

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science and make people discover it.

78

Sciences ACO is more than just a museum display-

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ing unique items. Thanks to the technical skills of its

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members and to the countless hours they spend on site,

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various working instruments are also presented to the

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public. The association has its own workshop adjacent

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to the display halls. Figure 3 shows a picture of this

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workshop during the maintenance of a ”cosmic arch”,

85

a device designed and built at LAL and which allows

86

the public to discover the angular distribution of cosmic

87

muons.

88

Figure 3: Maintenance of a ”cosmic arch” in the museum workshop.

2. Permanent exhibitions

89

2.1. The Pierre Marin hall

90

Pierre Marin (1927-2002) was a figure of the French

91

accelerator community, the ACO group leader and one

92

of the founding fathers of the Science ACO association.

93

After he passed away, his name was rightfully given to

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the large hall with thick concrete walls which houses the

95

ACO collider – see Fig. 4. Visitors can go around the

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machine to look at its different components (injection,

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dipole and quadrupole magnets, RF cavity, vacuum sys-

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tem, interaction region, see Fig. 5) which are still part of

99

today’s colliders or storage rings. In some sense, ACO

100

can be considered as an ”ancestor” of the CERN LHC.

101

Figure 4: The ACO collider in the Pierre Marin hall ( cClaude Men- neglier).

In addition to the ACO collider, various devices

102

are on display in this exhibition room: detector orig-

103

inal pieces belonging to the H1 [7] and NEMO-3 [8]

104

experiments, educational experiments (cloud chamber,

105

Helmholtz coils, cosmic arch, etc.) and a synchrotron

106

beamline rebuilt using real historical components.

107

2.2. The control room of the former LAL linear accel-

108

erator

109

A new room was opened in the museum in Septem-

110

ber 2013 to display the control room of the former LAL

111

linac. The actual exhibition, seen in Fig. 6, is not an

112

exact replica of the original setup of the control room

113

but uses optimally the available space to give the visi-

114

tors the best experience made possible by this historical,

115

scientific and technological display. This record of the

116

seventies allows the Sciences ACO guides not only to

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explain how this machine was operated and what its per-

118

formances were, but also to shed light on the extraordi-

119

nary advances of electronics and computing since then.

120

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Figure 6: The LAL linac control room, on display at the Sciences ACO museum since September 2013.

Interaction region RF cavity

Vacuum system Injection

Figure 5: Schematics of the ACO ring seen from above, with its main components highlighted.

This exhibit was achieved after years of lobbying,

121

first to preserve this room from disassembly and then

122

to have it moved to Sciences ACO. And this project

123

could not have been successful without the dedication

124

of Henri Borie who has been on the front line since the

125

beginning of this struggle. The association is currently

126

working on producing supporting material for this new

127

room: a leaflet and various multimedia resources.

128

2.3. The Electron Ronde

129

The Electron ronde, designed and built by the Sci-

130

ences ACO association, is probably the world’s smallest

131

interactive electron ring model. It includes a table-top

132

10 keV electron linac in which electrons are injected

133

Figure 7: The Electron ronde.

by a Minitel2 gun. The diameter of its ring, shown in

134

Fig. 7, is about 50 cm and the electron trajectory is vis-

135

ible thanks to the helium gas which is injected in the

136

vacuum tube. Magnets of variable strengths show how

137

the electromagnetic fields act on charged particles and

138

how these properties are used to steer a beam in an ac-

139

celerator.

140

This unique equipment is requiring careful operation

141

as it is a prototype whose design is still being optimized.

142

Yet, it has been on display during a two-week CNRS ex-

143

hibition near the Eiffel Tower in 2011 and should also be

144

shown in 2015 at the famous ”Palais de la D´ecouverte”

145

science museum in Paris.

146

2The ”Minitel” was a French text-only online service to which end users could connect through telephone lines, using a computer termi- nal of which millions of copies were produced. This service can be seen as a precursor of the World Wide Web.

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/Nuclear Physics B Proceedings Supplement 00 (2014) 1–6 5

3. Education and outreach activities

147

The Sciences ACO association is involved in many

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education and outreach activities whose target ranges

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from high-school students to the general public. One

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such activity which is worth mentioning is a weekly sci-

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ence club for a dozen of local school kids which ran for

152

three years in a row: it was an introduction to every-

153

day physics with a different topic for each session, illus-

154

trated by experiments whose results were used to under-

155

stand properties of the underlying phenomena. Another

156

example is a treasure hunt in the ”Valley of accelera-

157

tors”, organized every year during the open day of the

158

national science festival: participants are given a map of

159

the Orsay campus in which open sites hosting a particle

160

accelerator are highlighted. At each stage they have to

161

solve an enigma or answer some questions. A Kinect-

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based computer game was also developed in association

163

with the local Engineer School ”Polytech Paris-Sud [9]:

164

the player’s goal is to make two particle beams collide.

165

Finally, more common outreach activities are also of-

166

fered by the association: public lectures, display of ed-

167

ucational experiments, participation in science and so-

168

ciety debates (e.g. about nuclear energy), etc. Locally,

169

Sciences ACO is also one of the main driving forces of

170

education projects on the campus of the future Paris-

171

Saclay Higher Education Complex.

172

As already mentioned above, Sciences ACO is re-

173

ally focused on documenting its exhibitions. Various

174

brochures are available for visitors while additional ma-

175

terial can be downloaded from the website. Moreover,

176

the association managed to draw technology experts’ at-

177

tention to its museum: two virtual visits are currently

178

being developed – see Fig. 8.

179

• The first one is based on an online virtual

180

world and is created by a high-school physics

181

teacher from Strasbourg, Pierre Wild, and his stu-

182

dents [10]. Ultimately, it could allow to simulate a

183

particle injection into ACO, steered from the con-

184

trol room of the linac.

185

• The other uses 360-degree high resolution pictures

186

on which links can be superimposed to navigate in

187

the museum, open explanatory popup texts, watch

188

videos, etc. This functionality [11] is provided by

189

Sylvain Crouzier from the Paris-Sud University.

190

4. Prospects and challenges

191

Since its founding more than 20 years ago, the asso-

192

ciation always had to fight against limited resources –

193

both in terms of manpower and money. It benefits from

194

Figure 8: Example screenshots of the Sciences ACO virtual visits.

Top: a visit included in an online virtual world; bottom: a visit based on high resolution pictures (here a view of the ACO ring from the top, using a ”mini planet” projection mode).

the support of many partners and institutions: the LAL

195

and SOLEIL laboratories; the Paris-Sud University; the

196

department (Essonne) and the region (Ile-de-France);

197

the two neighboring cities Bures-sur-Yvette and Orsay;

198

finally the CNRS/IN2P3.

199

While extending the size of its exhibition and improv-

200

ing the items on display, Sciences ACO is facing several

201

recurring problems. First, its premises are falling into

202

disuse and require extensive (and expensive!) refurbish-

203

ment. Then, the facility is still classified as nuclear in-

204

stallation and hence its access is strictly controlled; in

205

particular, all visits must be cleared in advance. This is-

206

sue may be fixed in the near future if the museum main

207

piece, namely the ACO storage ring (whose decommis-

208

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sioning was achieved years ago) could be ”administra-

209

tively decoupled” from the linac areas which are still

210

radioactive (and closed to the public). Finally, Sciences

211

ACO is a remote museum, located on a university cam-

212

pus, which needs to be advertised again and again to

213

attract local people.

214

0 1 2 3 4 5 6 7 8

<25 25-35 35-45 45-55 55-65 65-75 75-85 >85

Sciences ACO membership [according to age]

Age

Figure 9: Distribution of the age of the active Sciences ACO members.

A key challenge ahead for the association is shown in

215

Fig. 9: the age distribution of the association members

216

is peaking above 70 years old. To strengthen the work

217

done so far and continue to grow, Sciences ACO has

218

to recruit new and younger members who will take over

219

from the generation who worked on the storage ring and

220

had the idea to turn this machine into a museum.

221

5. Conclusions

222

The Sciences ACO Light and Matter Museum is a

223

special place to talk about the history of science and

224

technology over more than four decades. Fueled by the

225

enthusiasm and the energy of the members of the asso-

226

ciation, it displays several rare (if not unique) museog-

227

raphy elements, among which the ACO collider and the

228

control room of the former LAL linac. Hundreds of peo-

229

ple, from school students to the general public, visit its

230

exhibitions every year and can see home-made educa-

231

tional experiments, like the ”Electron Ronde”.

232

All of this has been obtained by a small group of ded-

233

icated individuals, within the limited financial resources

234

of the association and an essential institutional support.

235

In spite of its past and present achievements, Sciences

236

ACO will have to find ways of renewing its membership

237

in order to amplify its educational and cultural impact.

238

Acknowledgment

239

Sciences ACO wishes to thank its long term part-

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ners whose support is essential to the running of the

241

association: the LAL and SOLEIL laboratories; the

242

Paris-Sud University; the department (Essonne) and

243

the region (Ile-de-France); the two neighboring cities

244

Bures-sur-Yvette and Orsay; finally, the CNRS/IN2P3.

245

The association would also like to thank the ”Unit´e

246

d´emant`element de l’installation nucl´eaire de base 106

247

(LURE)” (UDIL) for its help and support to run the Sci-

248

ences ACO museum during the past decade.

249

References

250

[1] Sciences ACO,http://www.sciencesaco.fr.

251

[2] P. Marin, Un demi-sicle d’acc´el´erateurs de particules, Dauphin,

252

2009.

253

[3] N. Arnaud, J. Ha¨ıssinski, The LAL-LURE accelerator complex,

254

a new EPS historic site, Europhysicsnews 44 (6) (2013) 4–5.

255

[4] Laboratoire de l’Acc´el´erateur Lin´eaire, http://www.lal.

256

in2p3.fr.

257

[5] SOLEIL Synchrotron, http://www.synchrotron-soleil.

258

fr/portal/page/portal/Accueil.

259

[6] C. Bernardini, AdA:The first electron-positron col-

260

lider, Phys.Perspect. 6 (2004) 156–183. doi:10.1007/

261

s00016-003-0202-y.

262

[7] The H1 experiment at HERA,http://h1.desy.de.

263

[8] The Neutrino Ettore Majorana Observatory, http://nemo.

264

in2p3.fr.

265

[9] Polytech Paris-Sud, http://www.polytech.u-psud.fr/

266

fr/index.html.

267

[10] See for instance http://www.dailymotion.com/video/

268

x1yq339_jeux-serieux-astroparticules-2014_

269

school.

270

[11] Visites virtuelles de l’Universit´e Paris-Sud, http:

271

//www.visites-virtuelles.u-psud.fr/?s=pano42&s=

272

pano111&h=32&v=0&f=90.

273

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