CLEOPATRA
  • INTRODUCTION TO Cleopatra
    • šŸ‘‘What is Cleopatra?
      • ⚫Why Mantle?
    • šŸ«‚Our Partners
    • ā˜Æļøve(3,3) Fundamentals
      • Dilution Protection (Rebase)
      • V1 Gauge Boosts
      • veCLEO (veCLEO)
        • šŸ’°veCLEO Revenue Distribution Schedule
    • šŸ”®DEX Functionalities
      • Swaps
        • šŸŽ‹Swap Fee Structure
      • Voting
      • Bribing
      • Vesting (veNFT Management)
      • LP Staking
  • Concentrated Liquidity Core
    • šŸ¤”Concentrated Liquidity
      • šŸ”¢Fee Tiers
      • 🦭Fee Distribution
    • šŸ†CL Gauges
    • šŸ“œBUSL-1.1 License
    • šŸCompetitive Farming
  • CLEO Tokenomics
    • šŸ“ŠCLEO Token Distribution
    • šŸ“ˆEmissions Schedule
    • āŒxCLEO
      • How is xCLEO obtained?
      • How is xCLEO used?
      • ā˜øļøxCLEO "Flywheel"
    • šŸŒ€Dilution Protection (3,3) Rebases
      • Partner Rebases
    • šŸ’§CLEO LGE - Liquidity Generation Event
      • LGE Specifics
  • Resources
    • šŸ“„Deployed Contract Addresses
    • šŸ“±dApp and Socials
    • šŸ“øCleopatra Media Kit
    • šŸŒ‰Bridging To Mantle
  • Security and Legal Considerations
    • šŸ›Fixed Solidly Vulnerabilities
    • šŸ› ļøWhy Proxy Contracts?
    • šŸ”Contract Timelock
    • šŸ˜ŽInherited Security
    • šŸ–‹ļøFormal Audits
    • āš–ļøRisks and Legal Disclosures
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  1. CLEO Tokenomics

Emissions Schedule

The liquid CLEO 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 the main priority.

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

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

The formula to calculate an Epoch's emissions is:

Emissions(t)=E0Ā āˆ—Ā (eāˆ’rt)Ā t=EpochsE0=Xāˆ’r=decayĀ coefficientEmissions{(t)} = E_{0}\ *\ (e^{-rt}) \\ \ \\ t = Epochs \\ E_{0} = X \\ -r = decay \ coefficientEmissions(t)=E0ā€‹Ā āˆ—Ā (eāˆ’rt)Ā t=EpochsE0​=Xāˆ’r=decayĀ coefficient

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

Emissions(epoch(N))Ā =Emissions(Nāˆ’1)Ā āˆ—(1.00āˆ’decay)Emissions(epoch(N)) \ = Emissions(N-1) \ * (1.00-decay)Emissions(epoch(N))Ā =Emissions(Nāˆ’1)Ā āˆ—(1.00āˆ’decay)
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Last updated 1 year ago

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