A Conjecture on the Minimal Size of Bound States
arXiv:1912.09485 · doi:10.21468/SciPostPhys.8.4.058
Abstract
We conjecture that, in a renormalizable effective quantum field theory where the heaviest stable particle has mass , there are no bound states with radius below (Bound State Conjecture). We are motivated by the (scalar) Weak Gravity Conjecture, which can be read as a statement forbidding certain bound states. As we discuss, versions for uncharged particles and their generalizations have shortcomings. This leads us to the suggestion that one should only constrain rather than exclude bound objects. In the gravitational case, the resulting conjecture takes the sharp form of forbidding the adiabatic construction of black holes smaller than . But this minimal bound-state radius remains non-trivial as , leading us to suspect a feature of QFT rather than a quantum gravity constraint. We find support in a number of examples which we analyze at a parametric level.
arXiv comment42 pages, 7 figures; v2: references added; v3: comments added
References in corpus (69)
- Theory of Bose-Einstein condensation in trapped gases
- The String Landscape, Black Holes and Gravity as the Weakest Force
- Quantum Resource Theories
- On the Geometry of the String Landscape and the Swampland
- The Swampland: Introduction and Review
- Dynamics of collapsing and exploding Bose-Einstein condensates
- Mass-radius relation of Newtonian self-gravitating Bose-Einstein condensates with short-range interactions: I. Analytical results
- The String Landscape and the Swampland
- On the metastability of the Standard Model vacuum
- Infinite Distances in Field Space and Massless Towers of States
- Proca Stars: gravitating Bose-Einstein condensates of massive spin 1 particles
- Solitons in the supersymmetric extensions of the Standard Model
- Pseudo-Stable Bubbles
- (Quantumness in the context of) Resource Theories
- Tensionless Strings and the Weak Gravity Conjecture
- Bose-Einstein Condensate general relativistic stars
- Naturalness and the Weak Gravity Conjecture
- The Weak Gravity Conjecture and Scalar Fields
- Small Q balls
- Dilute and dense axion stars
- The Symplectic Structure of N=2 Supergravity and its Central Extension
- Transplanckian axions !?
- A Stringy Test of the Scalar Weak Gravity Conjecture
- Natural Inflation and Quantum Gravity
- Boson Stars in AdS
- Planckian Axions and the Weak Gravity Conjecture
- New physics in a nutshell, or Q-ball as a power plant
- Dense Axion Stars
- Boson Stars from Self-Interacting Dark Matter
- Weak Gravity Strongly Constrains Large-Field Axion Inflation
- Black hole formation from axion stars
- Phase transitions between dilute and dense axion stars
- Repulsive Forces and the Weak Gravity Conjecture
- Constraints on Axion Inflation from the Weak Gravity Conjecture
- Collapse of Axion Stars
- Phase transitions precipitated by solitosynthesis
- The Weak Gravity Conjecture and Effective Field Theory
- Stable Phases of Boson Stars
- On Longevity of I-ball/Oscillon
- Large-Field Inflation with Multiple Axions and the Weak Gravity Conjecture
- Scalar Fields, Hierarchical UV/IR Mixing and The Weak Gravity Conjecture
- Warping the Weak Gravity Conjecture
- Axion boson stars
- Q-balls: Some Analytical Results
- Modulated Natural Inflation
- On charged boson stars
- Charged Proca Stars
- A Strong Scalar Weak Gravity Conjecture and Some Implications
- A Bound on Massive Higher Spin Particles
- Spinning boson stars and Kerr black holes with scalar hair: the effect of self-interactions
- Global view of QCD axion stars
- Moduli Stars
- Compact Boson Stars
- Stability of Q-balls and Catastrophe
- On Approximation Methods in the Study of Boson Stars
- Aligned natural inflation with modulations
- On Profiles of Boson Stars with Self-Interactions
- How does gravity save or kill Q-balls?
- Off-equilibrium infrared structure of self-interacting scalar fields: Universal scaling, Vortex-antivortex superfluid dynamics and Bose-Einstein condensation
- Chameleon stars
- Relativistic collapse of axion stars
- Bound states of the model via the nonperturbative renormalization group
- Relating the scalar weak gravity conjecture and the swampland distance conjecture for an accelerating universe
- A variational study of bound states in the Higgs model
- Large Field Inflation and Gravitational Entropy
- Fundamental Forces and Scalar Field Dynamics in the Early Universe
- A Species or Weak-Gravity Bound for Large Gauge Theories Coupled to Gravity
- Compact objects and the swampland
- Is Gravity the Weakest Force?
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- Pair Production and Gravity as the Weakest Force
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- Closed Strings and Weak Gravity from Higher-Spin Causality
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