The Arrows of Time: Orthogonal Book Three

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getting a
surprise on the turn.’
    ‘Hmm.’ Medoro had run out of ways to needle her.
    Serena gestured at the food in front of them. ‘We’ve all been stuffing ourselves, so don’t be shy about catching up.’ Agata took a spiced loaf from the table. She
hadn’t been able to eat with Cira in the apartment; every bite she took in her mother’s presence made her feel as if she were betraying her starving dead grandmother – who
hadn’t actually starved for long, and whose co had helped her raise her machine-fathered daughter.
    Vala asked Agata how her research was progressing.
    ‘Still slowly,’ Agata confessed.
    Gineto hummed sympathetically. ‘What is it exactly that you’re doing? Medoro’s tried to describe it to us, but I’m not sure he really understands it himself.’
    ‘I’m just a humble instrument builder,’ Medoro said. ‘You can’t expect me to begin to comprehend Agata’s work.’
    Agata ignored his teasing, but Gineto seemed genuinely curious. And if he wasn’t, he was being too polite to be brushed off with ‘it’s complicated’.
    She said, ‘Do you know about Lila’s work?’
    ‘Vaguely,’ Gineto replied. ‘Didn’t she find a way to make gravity compatible with rotational physics?’
    ‘Exactly. Vittorio’s law of gravity assumed absolute time. Yalda must have known that it wasn’t rotationally invariant, but in those days the discrepancy wasn’t seen as
important. People were busy enough trying to understand light.’
    ‘So . . . what changes?’ Gineto asked. ‘What does Vittorio’s inverse square law become?’
    ‘It’s trickier than that,’ Agata warned him. ‘In Lila’s theory, gravity isn’t a force at all, in the traditional sense: it’s a result of four-space
being curved. You know how lines of longitude on a globe come together? Even though they start out parallel at the equator, they don’t remain the same distance apart.’
    ‘Right,’ Gineto agreed tentatively. There was nothing esoteric in the geometry she’d described, but he couldn’t quite see the connection.
    Agata said, ‘In Lila’s theory, gravitational attraction is the same kind of effect. When two massive bodies start out at rest with respect to each other – that is, with their
histories parallel – they don’t stay the same distance apart, they accelerate towards each other. But you don’t need a force for that; all you need is curvature.’
    Gineto buzzed: he got it now. ‘That’s an elegant idea. Have the astronomers tested it?’
    ‘That’s the hardest part,’ Agata admitted. ‘The mathematics is beautiful, but we’re so far from any truly massive bodies that it’s almost impossible to devise
a test.’
    ‘The ideal thing to study would be a planet orbiting close to its star,’ Medoro interjected. ‘Like the innermost planet in the home system. What was that called? Paolo? Peleo?
I can never quite remember it.’
    Agata said, ‘Lila’s theory predicts that a close elliptical orbit would undergo “apsidal precession”: the near and far points of the orbit should move around the star,
instead of staying fixed in space. So careful observations of a system like that could distinguish her theory from Vittorio’s.’ She sketched an example on her chest.
     

    ‘If there are other planets in the system it’s more complicated,’ she added. ‘The way they tug on each other will cause precession, too, so you have to
separate out the various contributions. If we had copies of all the ancestors’ astronomical measurements we could hunt for some sign of Lila’s precession, but nobody thought to include
that kind of thing in the library.’
    ‘And where does your own work fit into all this?’ Gineto pressed her.
    ‘My work’s about trying to understand entropy in the context of Lila’s theory,’ Agata replied. ‘According to Lila, the curvature of four-space depends on both the
amount of matter present and the way it’s moving. If all the particles’

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