Stringy Microstates: Beyond the Black Hole Horizon
New research unveils a supersymmetric solution describing highly excited strings, offering a potential pathway to understanding the quantum nature of black holes without invoking a traditional event horizon.
![Black hole evaporation proceeds via a beam splitter mechanism coupled with single-mode squeezing for each interaction event, indexed by integer [latex]k[/latex], fundamentally altering the understanding of Hawking radiation.](https://arxiv.org/html/2601.09820v1/x3.png)
![The study elucidates dark matter-nucleon scattering and the decay of eta mesons into two pions via a scalar resonance, demonstrating that the coupling strength [latex]g_{u}(g_{\chi})[/latex] - and its effective counterpart [latex]g_{N}[/latex] as defined in equations (3) and (5) respectively - fundamentally governs these interactions.](https://arxiv.org/html/2601.10597v1/x701.png)
![The study demonstrates how cavity-mediated interactions sculpt the behavior of two-body wavefunctions, revealing distinct ground states-either spatially extended for repulsive interactions at strengths of [latex]V_0 = 10\varepsilon[/latex] and [latex]V_0 = 100\varepsilon[/latex], or localized for the corresponding attractive cases-as dictated by the second term of Eq. (II.2).](https://arxiv.org/html/2601.10301v1/x1.png)
![The distributions of [latex]\pi^+ \pi^-[/latex] and [latex]K_S^0 K_S^0[/latex] pairs are modeled with relativistic Breit-Wigner functions to identify resonance peaks, while a smoothly varying function accounts for residual background, effectively distinguishing signal from noise in the data.](https://arxiv.org/html/2601.09777v1/x6.png)

