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1 The Tight Knot Spectrum in QCD Tom Kephart Vanderbilt University Seminar at the University of Edinburgh 10 October 2012

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Page 1: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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The Tight Knot Spectrum in QCD

Tom Kephart Vanderbilt University

Seminar at the University of Edinburgh

10 October 2012

Page 2: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Knots, Links, and Physics

Examples of Knots and Links in Physics

Knots and Tight Knots: Theory

Tight Knots/Links in QCD

Other Possible Tight Knot Applications

Page 3: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Introduction: Tight Knots and Physics

● Many Potential Physical Systems can be Knotted or Linked, some tightly

● Examples in Several Areas of Physics

Page 4: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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List of ExamplesCLASSICAL PHYSICS/BIOPHYSICS● Plasma Physics● DNA● MacroBiology

QUANTUM PHYSICS● QCD Flux Tubes (tight)● Superconductors (tight)● Superfluids and Superfluid Turbulence● Atomic Condensates● Cosmic Strings (tight?)

UNIVERSALITY for Tight Quantum Case

Page 5: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Plasma Phys: Magnetic Flux Tubes● Tubes under Tension Contract● Minimum Length Determined by Topology● Taylor States in Plasma● Differs for QCD where radius is fixed

A. Stasiak, et al., Nature 384, 122 (1996)

L. Woltjer, PNAS, 44, 489 (1958)Plasma Physics

Biology

H. K. Moffatt, J. Fluid Mech. 35, 117 (1969)J. B. Taylor, PRL, 33, 1139 (1974)

Page 6: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Plasma Physics: SOHO images

Page 7: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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See e.g., P. M. Bellan, ``Spheromaks,’’ (2000)

Page 8: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Knot / Link stabilty

Conserved quantum numbers

Gaussian linking--Hopf link, trefoil knot

Genealized linking--Borromean rings, etc.

Page 9: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Tightly Knotted DNA

Tight knots first discussed and lengths estimated in:

Katritch, V., Bednar, J., Michoud, D., Scharein, R.G., Dubochet, J. & Stasiak, A. (1996) Nature

Katritch, V., Olson, W.K., Pieranski, P., Dubochet, J. & Stasiak, A. (1997) Nature.

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Page 11: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Page 12: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Flux Tubes in Quantum Chromodynamics

● Glueballs as Tight Knots and Links ● Quantized Flux● Knot “Energy” (EK = L/r) Length

Proportional to Particle Mass● Semi-classical model at the level of

liquid drop model of nucleus or QCD bag model

Page 13: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Tight Knots and Links in QCD

T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient Descent,” arXiv:1002.1723

Roman V. Buniy and TWK, “A model of glueballs,’’ Phys. Lett. B576, 127 (2003)

R. Buniy and TWK,“Glueballs and the universal energy spectrum of tight knots and links,’’ Int. J. Mod. Phys. A20, 1252 (2005)

R. Buniy, J. Cantarella, TWK and E. Rawdon,“The tight knot spectrum in QCD,” arXiv:1212.xxx

Page 14: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Chromoelectric Flux

● Flux between q, qbar pair is chromoelectric● Open for normal mesons● Closed in our case● Knotted and/or linked

Page 15: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Page 18: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Page 20: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Counting knotsn = number of crossings

Hoste et al. 1998N. Sloane, The On-Line Encyclopedia of Integer Sequences!

Page 21: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Types of knots and links

● Prime knots● Composite knots (connected sums of

prime knots)● Prime links ● Composite links● Physics should allow all types !

Page 22: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Non-q-qbar bosonic hadrons

Page 23: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Glueballs● Hadrons - Strong Interactions● No Valence Quarks, fJ states (JPC = J++)● Do not Decay Directly to Photons

● Decay in Knotted Flux Tube Model of Glueballsvia QM processes:

1. String (Tube) Breaking 2. Reconnection 3. Tunneling

Page 24: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Page 27: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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2012 Refit with New Data● New Glueball Data JPC = J++ States

Particle Data Group 2011● New Tight Prime Knot/Link Data● New! Composite Knots and Links● Expect continuum of glueballs by

~3 GeV from knot counts

R. Buniy, J. Cantarella, TWK and E. Rawdon,“The tight knot spectrum in QCD,” arXiv:1212.xxxx

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Curvature Corrections● We have physical knots, not ideal knots● Flux is uniform across cross sections of

straight tubes● But, knotted and linked tubes are curved● Flux is not uniform across cross sections of

curved tubes● Correct energy for curvature

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Page 33: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Toroidal Solenoid-Cross Section

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Curvature Correction as a Function of R2

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Page 37: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Page 38: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Histogram of the magnitudes of the curvature corrections to the first 72 knot and link lengths.

Page 39: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

39Histogram of the magnitudes of the curvature corrections to all 945 currently tabulated knot and link lengths.

Page 40: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Fit fJ's to knots

Curvature corrections included in fit

Page 41: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

41Knot Length

Glu

ebal

l Mas

s

Page 42: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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The Glueball Tartan

Glu

ebal

l Mas

s

Knot Length

Page 43: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Fit● We fit one set of sporadic numbers with

another● I.e., f-state masses <---> knot lengths● Either one-parameter: slope● Or two parameters: slope and intercept

Page 44: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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fJ's vs knot lengths

One parameter fit with uncorrected knot lengths

Page 45: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Options● Linear fit: 1-1 in order of mass/length● Move f states with large error bars out of

order to improve fit to:1. Account for tension in data by leaving gaps2. Find best fit

Page 46: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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fJ's vs knot lengths

One parameter fit with curvature corrected knot lengths

Page 47: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Best qualified fit

● This previous figure is best fit allowing for resolution of the tension in the data at ~1220 MeV

● Free knot i.e., 421 unassigned and used to

predict a state near 1200 MeV

Page 48: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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fJ's vs knot lengths

One parameter fit with curvature corrected knot lengths

Page 49: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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One parameter curvature corrected vs uncorrected fits

● f(1270) and f(1285) poorly fit without curvature correction

● Fit of f(1270) and f(1285) considerably improved with curv. correction

Page 50: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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fJ's vs knot lengths

Two parameter fit with uncorrected knot lengths

Page 51: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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fJ's vs knot lengths

Two parameter fit with uncorrected knot lengths

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Two parameter fits

● Two parameter fit does not pass through origin for no curv. correction

● Curv. Corrected two parameter fit is consistent with zero intercept

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Other Corrections

Toroidal flux tube (minor radius R1, major radius R2) constricting a cylindrical flux tube of radius R(z)

Page 54: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Other Corrections

Constriction

Balance tension with magnetic pressure

Estimate 5% correction for Hopf link

QCD may be more complicated—confinement effects, etc.

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Other Corrections

Distortion of tube cross section

E.g., wrap a rope tightly around a post and it'sCross section distorts

Estimate few % corrections

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Corrections to Knot Lengths● Curvaturecorrections ~ few % variation● Constriction corrections few %● Distortion corrections few %● QCD effects ?

● Conservative assumption:

3% error on knot energy● Note: only the spread in corrections is

important

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one parameter fit—curvature corrected

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Best unqualified fit

● The previous figure is the best overall fit● f(1350) was reordered

Page 59: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

59two parameter fit—curvature corrected

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Predictions for masses

Page 61: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

61Fit plus predictions

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Quality of the fit

Page 65: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Fit and predicted masses for 1st 22 knots/links

Page 66: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Predicted fJ's from knot energies

From one parameter fit with curvature corrected knot lengths

● No new states below ~1680 MeV (Not inconsistent with one new state at ~1195 MeV upon reording f(1370))

● Five new states 1690—1705 MeV range● Many new states above ~ 1720 MeV

● Estimated to 3% accuracy

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Comments about Predictions

● There is tension in the data near f(1710), f(1810), and some other high mass f-states.

● 50 years of HEP data to reconcile ● Multiple states possible in these regions● Attempts should be made to resolve them

Page 68: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Smallest knot on a cubic lattice

Minimal trefoil hits 24 vertices, Y. Diao (1993)

From knotplot, Rob Scharein

Page 69: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Trefoil energy

● Minimal lattice trefoil energy = 24● Minimal lattice trefoil energy ~ 16.44● Lattice could predict knot energies on the

high side

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Lattice

Conventional glueball on lattice--difficult problem

Lattice knotted and linked flux tubes--open problem

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CONCLUSIONS

CLASSICAL SYSTEMS ● Systems can Knot and Link ● Possibly Tight● Varying Tube Radius and

Energy Spectrum

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CONCLUSIONS

QUANTUM SYSTEMS ● Knots and Links● Fixed Tube Radius (Quantized Flux)● Tight implies “Quantized Lengths” for tight knots● Quantized Energy

● Universal Spectra

One Parameter per System - the SlopePredictions for QCD !

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END

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Now fit with only f0 data

More conservative

No interpretation of J > 0

Only 6 states, so more predictions

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75Knot energy vs glueball mass, 2003 results

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MeV

length

Fit of all fJ data of mass < 2 GeV/c2

(Assume all knots and links known)

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Data and Predictions for fJ States

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MeV

length

Model Predictions

~1210 MeV/c2

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79length

MeV

Fit of f0 data only

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MeV

length

Predictions from fit to f0 data

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Data and Predictions for f0 States

MeV

length

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The Tight Knot Spectrum in QCD

Tom Kephart Vanderbilt University

Presented at the Isaac Newton Institute

TOD Programme 17 November 2012

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The Tight Knot Spectrum in QCD

Tom Kephart Vanderbilt University

Presented at the International Centre for Mathematical Sciences

Edinburgh 3rd TOD workshop Isaac Newton Institute

17 October 2012

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Feeding Hagfish

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Results Knot Length Errors ~0.1% R2 = .9996 for n = 10 f0 States Slope Parameter S = 60.6 +/- 0.91 MeVIntercept -9.0 +/- 26.1 S ~ ΛQCD/π New States at E = EKxS

E.g., 41

2 at E = 1203 MeV, 77

2 at E = 1673 MeV, etc.

Page 88: The Tight Knot Spectrum in QCD - University of Edinburgh · Tight Knots and Links in QCD T. Ashton, J. Cantarella, M. Piatek, E. Rawdon,“Knot Tightening By Constrained Gradient

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Counting knots c chiral noninvertible + amphichiral noninvertible - amphichiral invertible i chiral invertible a fully amphichiral and invertible