Abstract
We study the radius of gyration \(R_T\) of a self-repellent fractional Brownian motion \(\left\{ B^H_t\right\} _{0\le t\le T}\) taking values in \(\mathbb {R}^d\). Our sharpest result is for \(d=1\), where we find that with high probability,
For \(d>1\), we provide upper and lower bounds for the exponent \(\nu \), but these bounds do not match.
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Here, we leverage the fact that for any \(\beta > 0\), the expression \(\beta ^{\gamma _1} T^{\gamma _2} \log (T)^{\gamma _3}\) behaves like \(T^{\gamma _2} \log (T)^{\gamma _3}\) for large T, where \(\gamma _1, \gamma _2, \gamma _3\) are arbitrary numbers, with the constraint that \(\gamma _2\) and \(\gamma _3\) cannot both be zero.
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L. C. and P. X. are partially supported by NSF grant DMS-2246850 and L. C. is partially supported by a collaboration Grant (#959981) from the Simons foundation.
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Appendix A: Fractional Brownian Motions and Girsanov Theorem
Appendix A: Fractional Brownian Motions and Girsanov Theorem
In this section, we present some preliminaries about stochastic calculus for fBm’s. For a more detailed account of this topic, we refer the interested readers to [21].
A d-dimensional stochastic process \(B^H = \left\{ \left( B^{H,1}_t,\dots , B^{H,d}_t\right) :t\in \mathbb {R}_+\right\} \) is a called a fraction Brownian motion (fBm) with the Hurst parameters \(H \in (0,1)\) on a probability space \((\Omega , \mathcal {F}, \mathbb {P})\), if
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(i)
\(B^{H,i}\), \(i=1,\dots ,d\), are independent;
-
(ii)
for each \(1\le i\le d\), \(\left\{ B^{H,i}_t :t \in \mathbb {R}_+\right\} \) is a centered Gaussian family with covariance
$$\begin{aligned} \mathbb {E} \left[ B^{H,i}_t B^{H,i}_s\right] = \frac{1}{2}\left( t^{2H} + s^{2H} - |t-s|^{2H}\right) . \end{aligned}$$
Without loss of generality, we can assume that the filtration \(\left\{ \mathcal {F}_t :t \in \mathbb {R}_+\right\} \) is the canonical filtration generated by \(B^H\).
Next, we define the integration of deterministic functions against fBm’s. If \(\phi \) is a smooth function on \(\mathbb {R}_+\) with compact support, i.e., \(\phi \in C_c^{\infty }(\mathbb {R}_+)\), then the integrals
are centered Gaussian random variables with the following covariance structure:
![](http://media.springernature.com/lw518/springer-static/image/art%3A10.1007%2Fs10955-023-03227-y/MediaObjects/10955_2023_3227_Equ75_HTML.png)
for all \(1\le i,j \le d\), and \(\phi , \psi \in C_c^{\infty }(\mathbb {R}_+).\)
By typical approximation arguments, one can extend the integration to the Hilbert space \(\mathcal {H}\) of functions on \(\mathbb {R}_+\), with inner product,
In particular, for any \(t\in \mathbb {R}_+\), the function \(w(t,\cdot )\), given by
is an element of \(\mathcal {H}\) (see [22, Proposition 2.1]), where, with \(B(\cdot ,\cdot )\) denoting the Beta function,
![](http://media.springernature.com/lw243/springer-static/image/art%3A10.1007%2Fs10955-023-03227-y/MediaObjects/10955_2023_3227_Equ76_HTML.png)
This observation allows us to define the following Gaussian process \(M = M^{\textbf{u}} = \{ M_t :t \in \mathbb {R}_+\}\) with parameter \(\textbf{u} = (u_1,\dots , u_d)\) being a unit vector in \(\mathbb {R}^d\) as follows:
The following theorem is a straightforward extension of [22, Theorem 3.1] from \(d=1\) to higher dimensional cases, thanks to the independence of the components of \(B^H\):
Theorem A.1
Let \(B^H\) be a d-dimensional fBm with \(H \in (0,1)\), let \(\textbf{u}\) be a unit vector in \(\mathbb {R}^d\), and let \(M = M^{\textbf{u}}\) be the Gaussian process given as in (3.1). Then M is a square-integrable martingale with quadratic variation
![](http://media.springernature.com/lw557/springer-static/image/art%3A10.1007%2Fs10955-023-03227-y/MediaObjects/10955_2023_3227_Equ77_HTML.png)
For any \(\lambda > 0\) and \(T > 0\), denote
and let \(\mathbb {P}_T^{\lambda } = \mathbb {P}_T^{\lambda , \textbf{u}}\) be a probability measure on \((\Omega , \mathcal {F}_T)\) that is equivalent to \(\mathbb {P}_T\) with the Radon–Nikodym derivative
The next theorem, a Girsanov formula for fBm’s, is a straightforward extension of [22, Theorem 4.1].
Theorem A.2
Under probability \(\mathbb {P}^{\lambda }_T\), the process \(\left\{ B^H_t :0 \le t \le T\right\} \) is a d-dimensional fBm with a drift \(\lambda \textbf{u}\in \mathbb {R}^d\), i.e., the distribution of the process \(B^H\) up to time T under \(\mathbb {P}^{\lambda }_T = \mathbb {P}^{\lambda ,\textbf{u}}_T\) is the same as \( B^{H, \lambda , \textbf{u}, T} = \left\{ B^H_t + \lambda t\, \textbf{u} \,:0\le t\le T\right\} \) under \(\mathbb {P}_T\).
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Chen, L., Kuzgun, S., Mueller, C. et al. On the Radius of Self-Repellent Fractional Brownian Motion. J Stat Phys 191, 19 (2024). https://doi.org/10.1007/s10955-023-03227-y
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DOI: https://doi.org/10.1007/s10955-023-03227-y