Back The Sandpit Save as PDF
Chapters (55)
  1. Cover
  2. About the Author
  3. Also by Nicholas Shakespeare
  4. Dedication
  5. Epigraph
  6. Prologue
  7. PART ONE
  8. Chapter One
  9. Chapter Two
  10. Chapter Three
  11. Chapter Four
  12. Chapter Five
  13. Chapter Six
  14. Chapter Seven
  15. Chapter Eight
  16. Chapter Nine
  17. Chapter Ten
  18. Chapter Eleven
  19. Chapter Twelve
  20. Chapter Thirteen
  21. Chapter Fourteen
  22. Chapter Fifteen
  23. Chapter Sixteen
  24. Chapter Seventeen
  25. Chapter Eighteen
  26. Chapter Nineteen
  27. Chapter Twenty
  28. PART TWO
  29. Chapter Twenty-one
  30. Chapter Twenty-two
  31. Chapter Twenty-three
  32. Chapter Twenty-four
  33. Chapter Twenty-five
  34. Chapter Twenty-six
  35. Chapter Twenty-seven
  36. Chapter Twenty-eight
  37. Chapter Twenty-nine
  38. Chapter Thirty
  39. PART THREE
  40. Chapter Thirty-one
  41. Chapter Thirty-two
  42. Chapter Thirty-three
  43. Chapter Thirty-four
  44. Chapter Thirty-five
  45. Chapter Thirty-six
  46. PART FOUR
  47. Chapter Thirty-seven
  48. Chapter Thirty-eight
  49. Chapter Thirty-nine
  50. Chapter Forty
  51. Chapter Forty-one
  52. Chapter Forty-two
  53. Chapter Forty-three
  54. Chapter Forty-four
  55. Acknowledgements

Until now, there had been no breakthrough in heating plasma to a ‘self-sustained burn’ – that is to say, to the point where the plasma generated more heat than was put into it, although there had been many experiments using exotic metals, super-conducting magnets, giant lasers and so forth.

Always, the instabilities got in the way.

In the south of France, the world’s most advanced nations had chosen to build a big expensive reactor costing $25 billion. But this wouldn’t be tested for another eight years. Even then, ITER could very well fail like the Zeppelin, or like the fission breeder reactor in America, fifteen years in the making, and closed down before it had conducted a single experiment.

Other than in a hydrogen bomb, which needed to be triggered by a fissile atomic explosion, the most successful attempt to replicate fusion peacefully on earth had been at the Culham laboratory outside Oxford: here, in 1997, in a gigantic machine the size of the Pompidou Centre, fusion had been achieved – if for less than a second. The trick was to keep fusion going for much longer, and on a vastly smaller scale, but this had eluded the world’s scientific community. Cold fusion, tokamaks, stellarators, magnetic confinement – each had held up a flickering promise. Not one device had proved to work. A self-sustained burn continued to stay out of reach, a chimera.

‘That is, until 7.32 p.m. last Friday.’

But Marvar was rushing ahead of himself. None of this would make sense unless Dyer understood the nature of his research.

‘Pauli? You have heard of him?’

Dyer admitted that he hadn’t.

‘Pauli was a pioneer of quantum physics,’ Marvar went on, with an erudite smile. ‘He was watching a revue at a theatre in Copenhagen when the exclusion principle came to him.’

Marvar had his brainwave after going to see Samir play at Summer Fields.

‘Do you know what gave me the idea?’ Marvar said, gathering momentum. ‘The football!’

In order to make the ‘burn’, you needed to squash atoms into incredibly high densities. ‘The problem is, it’s like wrapping your fingers around a party balloon and then trying to squeeze. The balloon squishes out between your fingers and you can’t do it.’ The only way of attaining fusion was to create an absolutely symmetrical profile. ‘We have never achieved coherence all the way round, that is to say a perfect spherical wavefront – like a wave arriving along the beach at the same time.’ At Livermore, where billions of dollars had been spent on this, an array of long multiple lasers each one the size of two football pitches were beamed onto a target pellet so minuscule that you almost couldn’t see it, and every single time there had been spots.

‘Spots means squishing. It means it is not symmetrical.’