Abstract
We establish the Lee–Huang–Yang formula for the ground state energy of a dilute Bose gas for a broad class of repulsive pair-interactions in 3D as a lower bound. Our result is valid in an appropriate parameter regime of soft potentials and confirms that the Bogoliubov approximation captures the right second-order correction to the ground state energy.
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Notes
Note that we allow but not require R to be smaller than \(\rho ^{-1/3}\).
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Acknowledgements
This project started out many years ago from a fruitful discussion with E. H. Lieb, who the authors are very grateful to. This work was primarily done in Copenhagen and the authors acknowledge support by ERC Advanced grant 321029 and by VILLUM FONDEN via the QMATH Centre of Excellence (Grant No. 10059). BB also gratefully acknowledges support from the DFG (Grant No. AOBJ 643360 KN 102013-1) and under Germany’s Excellence Strategy EXC-2181/1 – 390900948.
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Appendix A: Taylor Expansions for the Bogoliubov Integral
Appendix A: Taylor Expansions for the Bogoliubov Integral
The quadratic Hamiltonian and thus the integral \(\int h_0(k) \, {\mathrm {d}}k\) (see Lemma 4.4) plays an important role in this article. In this appendix, we will estimate this integral using Taylor approximations to various order on different regions. The resulting estimates are given in a general form as powers in n. This allows us in several lemmas to obtain bounds on the energy from bounds on n, respectively, to obtain bounds on n for states which have sufficiently low energy.
Throughout this appendix we will assume that \(n\ge 1\) and that the condition on \(n|{B} |^{-1}\) in Lemma 4.6 is satisfied, so that by Lemma 4.4 we have the lower bounds
and
1.1 A.1. Bounds for the Quadratic Part of \(H_B\)
We estimate the operator-valued integral \(\frac{1}{2}(2\pi )^{-3}\int h_0(k)\, {\mathrm {d}}k\) using the following facts.
Around \(x=0\) we can write \(\sqrt{1+x}=1+\frac{1}{2}x-\frac{1}{8}x^2+\frac{1}{16}x^3+O(x^4)\) yielding the bounds
If B is either a small or a large box, then, for all \(k\in {\mathbb {R}}^3\), the parentheses in (A.1) is positive.
This is easy to see. If B is a small box and \(|{k} |\le (ds\ell )^{-1}\), then \(\tau _B(k^2)=0\) and \(\widehat{W}(k)>0\) by (104) since \((ds\ell )^{-1}<R^{-1}\). For \(|{k} |>(ds\ell )^{-1}\) we have \(\tau _B(k^2)>0\) and apply (A.4). For the large box the claim is proven analogously. We may therefore replace \(n_0\) by n in (A.1) when bounding \(h_0\) from below such that
Provided \(\tau _B(k^2)>0\), we write
1.1.1 A.1.1. Estimates on the Small Box
\(\tau _B(k^2)=0\) if \(|{k} |<(ds\ell )^{-1}\) while \(\widehat{W}(k)>0\) if \(|{k} |<R^{-1}\). Since \(\sqrt{1+x}\ge 1\) if \(x\ge 0\), we have
Using (A.3) for \(2(ds\ell )^{-1}<|{k} |<R^{-1}\) and (A.4) for \(|{k} |>R^{-1}\) gives
Since \(\tau _B=(1-\varepsilon _0)[|{k} |-(ds\ell )^{-1}]_+^2\ge C|{k} |^2\) if \(|{k} |\ge 2(ds\ell )^{-1}\) and we have \(|{\widehat{W}(k)} |\le \widehat{W}(0)\le Ca\), it is easy to estimate the last term in (A.8)
The integral \(\int _{{|{k} |>2(ds\ell )^{-1}}}^{{}}\frac{\widehat{W}(k)^2}{\tau _B(k^2)}\, {\mathrm {d}}k\) is related to the second Born term, and we have to estimate it carefully. Recall that on the small box we have by (31) that \(v_R(x)\le W(x)\le v_R(x)(1+C(\frac{R}{d\ell })^2)\). Thus we have
Since \(v_R(x)=\frac{1}{R^3} v_{1}(\frac{x}{R})\), we have \(\widehat{v_R}(k)=\widehat{v_{1}}(Rk)\) and that
For \(f\in L^{\frac{6}{5}}({\mathbb {R}}^{3})\) a real space representation (see [21] Cor 5.10) followed by an application of the Hardy–Littlewood–Sobolev inequality gives
On the small box, we have for \(|{k} |>2(ds\ell )^{-1}\)
We use a Cauchy–Schwarz inequality, (A.10) and (A.12) to obtain the estimate
Using \(|{\widehat{W}(k)} |\le Ca\), gives
Combining (A.13), (A.14) and (A.15), we arrive at
In the last inequality, we used that the second term in (A.14) and the positive term \((1+C\varepsilon _0)\frac{1}{R}\int _{{|{k} |<2(ds\ell )^{-1}R}}^{{}}\frac{\widehat{v}_{1}(k)^2}{|{k} |^2}\, {\mathrm {d}}k\) by Condition 1 are bounded by the last term in (A.16).
1.1.2 A.1.2. Estimates on the Large Box
Recall that on the large box, we have \({\int \chi _B^2=|{B} |}\) and that
Hence, as in (A.7),
Analogously to (A.8), we have
The last term in (A.18) is estimated in the same way as the last term in (A.8)
By (30), we have \(v_R(x)\!\le \! W(x)\!\le \! v_R(x)(1\!+\!C(\!\frac{R}{\ell })^2)\!\). Thus, similarly to (A.14),
Similarly to (A.15), we have
Since
we have, similar to (A.16),
In the last inequality, we used that by Condition 1 the terms \(C\frac{aR}{\ell ^2}a\) and \(\int _{{|{k} |<(s\ell )^{-1}}}^{{}}\,\frac{\widehat{v}_{R}(k)^2}{|{k} |^2}\, {\mathrm {d}}k\) are bounded by the second to last term in (A.23).
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Brietzke, B., Solovej, J.P. The Second-Order Correction to the Ground State Energy of the Dilute Bose Gas. Ann. Henri Poincaré 21, 571–626 (2020). https://doi.org/10.1007/s00023-019-00875-3
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DOI: https://doi.org/10.1007/s00023-019-00875-3