Reply to A. Patrascioiu's and E. Seiler's comment on our paper "The two-phase issue in the O(n) non-linear sigma-model: a Monte Carlo study"
B. Alles, A. Buonanno, G. Cella

TL;DR
This paper is a response to comments on a previous Monte Carlo study of the two-phase issue in the O(n) non-linear sigma-model, clarifying and defending the original findings.
Contribution
It provides a detailed reply addressing critiques of the Monte Carlo analysis in the context of the two-phase problem in the O(n) sigma-model.
Findings
Clarifies the original Monte Carlo results
Addresses specific critiques raised by Patrascioiu and Seiler
Reinforces the validity of the initial conclusions
Abstract
We reply to a comment by A. Patrascioiu and E. Seiler appeared in hep-lat/9608138 on our paper hep-lat/9608002.
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Taxonomy
TopicsTheoretical and Computational Physics · Complex Systems and Time Series Analysis
IFUP-TH 56/96
September 1996
Reply to A. Patrascioiu’s and E. Seiler’s comment on our paper
The two-phase issue in the non-linear ** -model: a Monte-Carlo study**
B. Allés, A. Buonanno and G. Cella
Dipartimento di Fisica and INFN,
Piazza Torricelli 2, 56126 Pisa, Italy
Our paper [1] has motivated a comment [2] by A. Patrascioiu and E. Seiler which we reply in this note. The remarks in [2] concern three statements that the authors select from our paper:
i) “The results for support the asymptotic freedom scenario”.
The authors in [2] recall that at small the expansion is Borel summable [3]. No rigorous proof has been given concerning the behaviour of the series at large . In [2] it is not shown if our working ’s () lie in the “small” or “large” region when but at least we can say that if the results from our Monte Carlo data fit so nicely the predictions for the model (within few per mille for the mass gap and susceptibility predictions, see [4]) there is reasonable room to think that the exact model (what we simulate) has a critical point at and the set of predictions are correct. If our data had to agree with some prediction other than the set of predictions for the model then the small difference between our result for the mass gap and the P. Hasenfratz et al. [5] prediction, 0.5% (compared for instance to the difference of almost 30% between the and the predictions) would become an intriguing challenge. Considering it as an accident is a matter of feelings.
ii) “Assuming finite-size scaling (FSS), it has been shown that presents asymptotic scaling starting from ”.
This statement is true: Assuming FSS it has been shown that the model presents asymptotic scaling within few per cent at large correlation lengths. We are aware of the validity of whenever the limit holds, where is the lattice size and any correlation length, (see for instance [6]). For this reason we made our simulations at large values of the previous ratio, . Therefore the second comment of [2] does not apply to us.
iii) “The model with Symanzik action does not show KT behavior”.
Strangely enough we have not written this sentence in our paper [1]. Maybe the authors had in mind some of the following sentences that do appear in the paper:
- (1.)
“If the constancy of … is a genuine physical effect, then also for the Symanzik action we should see such a behaviour”. 2. (2.)
“… our data [for the ratio ] are not constant”. 3. (3.)
“… our data [for ] do not support either or ”.
(1.) The tree-level improved Symanzik action (although invented in the context) is as good as any other action for describing the models on the lattice and it does not assume the validity of . Both the Lipschitz action (see for instance [7]) and the Symanzik action are in the same universality class as the standard action.
(2.) Figure 1 in [1] clearly shows that the ratio is not constant, in contrast to what happens for the standard action [8]. We stress the fact that our data have better statistics. Clearly a similar high-statistics simulation for the standard action is worth doing.
(3.) We clearly say in [1] that the data for the mass, magnetic susceptibility and ratio for the model satisfy the predictions only within , [4]. This fact, together with point (2.), led us to conclude that our data do not support either or . We cannot say more than this for the model.
The reference list from the paper itself. Each links out to its DOI / PubMed record.
- 1[1] B. Allés, A. Buonanno and G. Cella, hep-lat/9608002.
- 2[2] A. Patrascioiu and E. Seiler, hep-lat/9608138.
- 3[3] J. Fröhlich, A. Mardin and V. Rivasseau, Commun. Math. Phys. 86 (1982) 87.
- 4[4] B. Allés, A. Buonanno and G. Cella, to appear on hep-lat.
- 5[5] P. Hasenfratz, M. Maggiore and F. Niedermayer, Phys. Lett. B 245 (1990) 522; P. Hasenfratz and F. Niedermayer, Phys. Lett. B 245 (1990) 529.
- 6[6] B. Allés, M. Beccaria and F. Farchioni, Phys. Rev. D 54 (1996) 1044.
- 7[7] A. Patrascioiu and E. Seiler, J. Stat. Phys. 69 (1992) 573.
- 8[8] A. Patrascioiu and E. Seiler, hep-lat/9508014.
