We analyze the modifications that a dense nuclear medium induces in the ⁎Ds0⁎(2317)± and Ds1(2460)±. In the vacuum, we consider them as isoscalar ⁎D(⁎)K and ⁎D‾(⁎)K‾ S-wave bound states, which are dynamically generated from effective interactions that lead to different Weinberg compositeness scenarios. Matter effects are incorporated through the two-meson loop functions, taking into account the self energies that the ⁎D(⁎), ⁎D‾(⁎), K, and K‾ develop when embedded in a nuclear medium. Although particle-antiparticle [⁎Ds0,s1(⁎)(2317,2460)+ versus ⁎Ds0,s1(⁎)(2317,2460)−] lineshapes are the same in vacuum, we find extremely different density patterns in matter. This charge-conjugation asymmetry mainly stems from the very different kaon and antikaon interaction with the nucleons of the dense medium. We show that the in-medium lineshapes found for these resonances strongly depend on their ⁎D(⁎)K/⁎D‾(⁎)K‾ molecular content, and discuss how this novel feature can be used to better determine/constrain the inner structure of these exotic states.
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Montesinos et al. (2024) studied this question.
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