REVIEW
Observer-independent quanta of mass and length
High Energy Physics - Theory · Submitted 16 Feb 2001 · 13 references
Pith's verdict: A short, honest DSR letter whose central one-line fixed-point check needs a typo corrected before a reader can reproduce it.
T0 · AI review
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Referee report
The paper
The paper claims
Using the κ-Poincaré dispersion relation, the paper constructs a modified special relativity in which the Planck mass is observer-independent and the speed of light diverges at a finite momentum.
The reading
Extended reading notes
Core claim
The central claim is that a modified special relativity built on the κ-Poincaré dispersion relation M_P²c⁴(1 - e^{-E/M_P c²})² - c²p² = 0 makes the Planck mass M_P the same for all inertial observers, because the boost action vanishes at p = M_P c, and that the same relation implies a minimal length L_P. If correct, this supplies an existence proof that an observer-independent mass scale can be embedded in a deformed relativity, and it suggests that the Planck-scale regime is Galilean rather than Lorentzian.
Load-bearing premise
The load-bearing premise is that the κ-Poincaré bicrossproduct boost action (Eq. 4) and its dispersion relation (Eq. 6) are the right deformation to impose. The observer-independence of M_P is then a fixed-point property of that specific algebra, not a consequence of the three postulates alone. As printed, Eq. 4 has a p² term with coefficient (1/2)M_P c, which is dimensionally inconsistent; the displayed check δp = 0 at p = M_P c only works with the standard 1/(2M_P c) coefficient. So the result rests on an algebra imported from Majid-Ruegg and Lukierski et al., with a typo in the printed boost that a reader must correct to reproduce the conclusion.
Original abstract
It has been observed recently by Giovanni Amelino-Camelia \cite{gac1, gac2} that the hypothesis of existence of a minimal observer-independent (Planck) length scale is hard to reconcile with special relativity. As a remedy he postulated to modify special relativity by introducing an observer-independent length scale. In this letter we set forward a proposal how one should modify the principles of special relativity, so as to assure that the values of mass and length scales are the same for any inertial observer. It turns out that one can achieve this by taking dispersion relations such that the speed of light goes to infinity for finite momentum (but infinite energy), proposed e.g., in the framework of the quantum $\kappa$-Poincar\'e symmetry. It follows that at the Planck scale the world may be non-relativistic.
The compiled record
The paper's own sentences, arranged, kept beside the review and separate from it. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.
The abstract, sentence by sentence
It has been observed recently by Giovanni Amelino-Camelia \cite{gac1, gac2} that the hypothesis of existence of a minimal observer-independent (Planck) length scale is hard to reconcile with special relativity. As a remedy he postulated to modify special relativity by introducing an observer-independent length scale. In this letter we set forward a proposal how one should modify the principles of special relativity, so as to assure that the values of mass and length scales are the same for any inertial observer. It turns out that one can achieve this by taking dispersion relations such that the speed of light goes to infinity for finite momentum (but infinite energy), proposed e.g., in the framework of the quantum $\kappa$-Poincar\'e symmetry. It follows that at the Planck scale the world may be non-relativistic.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | It has been observed recently by Giovanni Amelino-Camelia \cite{gac1, gac2} that the hypothesis of existence of a minimal observer-independent (Planck) length scale is hard to reconcile with special relativity. | background 1.00 | 0.03 | 0.03 | asserted 0.87 |
| s1 | As a remedy he postulated to modify special relativity by introducing an observer-independent length scale. | background 1.00 | 0.04 | 0.05 | asserted 0.97 |
| s2 | In this letter we set forward a proposal how one should modify the principles of special relativity, so as to assure that the values of mass and length scales are the same for any inertial observer. | contribution 1.00 | 0.74 | 0.25 | hedged possibility 0.36 |
| s3 | It turns out that one can achieve this by taking dispersion relations such that the speed of light goes to infinity for finite momentum (but infinite energy), proposed e.g., in the framework of the quantum $\kappa$-Poincar\'e symmetry. | method 0.68 | 0.48 | 0.23 | asserted 0.76 |
| s4 | It follows that at the Planck scale the world may be non-relativistic. | interpretation 0.96 | 0.72 | 0.43 | hedged possibility 0.99 |
What was examined, and what was not
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References
How the literature uses it
49 arXiv papers cite this in 63 sentences
Papers citing it · 21 sentences without a confident label
Compares with it 1 paper
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This distinguishing feature sets meVSL apart from traditional VSL models, which often assume or necessitate an explicit mechanism driving the evolution of the speed of light [ref] .
Revisiting Varying Speed of Light in Cosmology: Insights from the Friedmann-Lema\^itre-Robertson-Walker Metric · Introduction · 0.83
Cites it as support 1 paper
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Indeed boosting a four-momentum with an infinite boost parameter will lead to infinite energy but finite linear momentum with Planckian magnitude [ref] .
Quantum gravity phenomenology at the dawn of the multi-messenger era -- A review · Modified kinematic symmetries · 0.97
Cites it as background 36 papers
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Deformations of special relativity (DSR) [ref] allegedly make it possible to introduce an energy-dependent speed of light in position space while still preserving observer-independence.
Comment on arXiv:1007.0718 by Lee Smolin · Introduction · 0.98
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For this purpose we return here to the simple perspective and formalization of the first studies [ref] which noticed that some known deformations of relativistic symmetries, some of the ones studied within the “doubly-special relativity" research programme (see, e.g., Refs. [ref] ), could result in the property that coincidences of events established by nearby observers might not appear as coincidences of events in the coordinatization of spacetime by distant observers.
Modeling transverse relative locality · Introduction · 0.80
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The alternative possibility is a “deformation" of relativistic symmetries, in the sense of the “Doubly-Special Relativity" [ref] (DSR) scenario, which insists on a relativistic formulation of laws, as required by the first postulate, and confines all revisions of relativity to revisions of the second postulate.
Testing quantum-spacetime relativity with gamma-ray telescopes · Introduction · 0.91
Discussion
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