RA Exchange
  • INTRODUCTION TO RA
    • 👑What is RA?
      • ✖️Why Fraxtal?
    • 🫂Our Partners
    • ☯️ve(3,3) Fundamentals
      • Dilution Protection (Rebase)
      • veRA (veNFT) [WIP]
        • 💰veRA Revenue Distribution Schedule
    • 🔮DEX Functionalities
      • Swaps
        • 🎋Swap Fee Structure
      • Voting
      • Bribing
      • Vesting (veNFT Management)
      • LP Staking
  • Concentrated Liquidity Core
    • 🤔Concentrated Liquidity
      • 🔢Fee Tiers
        • 🥢Tickspacings
      • 🦭Fee Distribution
    • 🏆CL Gauges
    • 📜BUSL-1.1 License
    • 🏁Competitive Farming
  • RA Tokenomics
    • 📊RA Initial Token Distribution [WIP]
    • 📈Emissions Schedule [WIP]
    • ❌xRA [WIP]
      • How is xRA obtained?
      • How is xRA used?
      • ☸️xRA "Flywheel"
    • 🌀Dilution Protection (3,3) Rebases
  • Resources
    • 📄Deployed Contract Addresses
    • 📱dApp and Socials
    • 📸RA Media Kit [WIP]
    • 🌉Bridging To Fraxtal
  • Security and Legal Considerations
    • 🐛Fixed Solidly Vulnerabilities
    • 🛠️Why Proxy Contracts?
    • 🔐Contract Timelock
    • 😎Inherited Security
    • 🖋️Formal Audits
    • ⚖️Risks and Legal Disclosures
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  1. RA Tokenomics

Emissions Schedule [WIP]

The liquid RA emissions according to the protocol's tokenomics

100% of ALL emissions go to gauges, there are no team emissions or other distributions. Full decentralization of the emission distribution is a core feature.

There is a 1% exponential decay week over week, reducing emissions in perpetuity.

The emissions schedule will be adjusted up and/or down based on market demand, to prevent over/under inflation in order to stay competitive.

The formula to calculate an Epoch's emissions is:

Emissions(t)=E0 ∗ (e−rt) t=EpochsE0=X−r=decay coefficientEmissions{(t)} = E_{0}\ *\ (e^{-rt}) \\ \ \\ t = Epochs \\ E_{0} = X\\ -r = decay \ coefficientEmissions(t)=E0​ ∗ (e−rt) t=EpochsE0​=X−r=decay coefficient

Alternatively, a user can calculate the emissions for an epoch based on the previous, as such:

Emissions(epoch(N)) =Emissions(N−1) ∗(1.00−decay)Emissions(epoch(N)) \ = Emissions(N-1) \ * (1.00-decay)Emissions(epoch(N)) =Emissions(N−1) ∗(1.00−decay)
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Last updated 1 year ago

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