Description:
<jats:title>Abstract</jats:title><jats:p>Brane world models have shown to be promising to understand the late cosmic acceleration, in particular because such acceleration can be naturally derived, mimicking the dark energy behaviour just with a five dimensional geometry. In this paper we present a strong lensing joint analysis using a compilation of early-type galaxies acting as a lenses, united with the power of the well studied strong lensing galaxy cluster Abell 1689. We use the strong lensing constraints to investigate a brane model with variable brane tension as a function of the redshift. In our joint analysis we found a value <jats:inline-formula><jats:alternatives><jats:tex-math>$$n = 7.8^{+0.9}_{-0.5}$$</jats:tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML">
<mml:mrow>
<mml:mi>n</mml:mi>
<mml:mo>=</mml:mo>
<mml:mn>7</mml:mn>
<mml:mo>.</mml:mo>
<mml:msubsup>
<mml:mn>8</mml:mn>
<mml:mrow>
<mml:mo>-</mml:mo>
<mml:mn>0.5</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>+</mml:mo>
<mml:mn>0.9</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:mrow>
</mml:math></jats:alternatives></jats:inline-formula>, for the exponent related to the brane tension, showing that <jats:italic>n</jats:italic> deviates from a Cosmological Constant (CC) scenario (n=6). We obtain a value for the deceleration parameter, <jats:italic>q</jats:italic>(<jats:italic>z</jats:italic>) today, <jats:inline-formula><jats:alternatives><jats:tex-math>$$q(0)=-1.2^{+0.6}_{-0.8}$$</jats:tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML">
<mml:mrow>
<mml:mi>q</mml:mi>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mn>0</mml:mn>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>=</mml:mo>
<mml:mo>-</mml:mo>
<mml:mn>1</mml:mn>
<mml:mo>.</mml:mo>
<mml:msubsup>
<mml:mn>2</mml:mn>
<mml:mrow>
<mml:mo>-</mml:mo>
<mml:mn>0.8</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>+</mml:mo>
<mml:mn>0.6</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:mrow>
</mml:math></jats:alternatives></jats:inline-formula>, and a transition redshift, <jats:inline-formula><jats:alternatives><jats:tex-math>$$z_t=0.60\pm 0.06$$</jats:tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML">
<mml:mrow>
<mml:msub>
<mml:mi>z</mml:mi>
<mml:mi>t</mml:mi>
</mml:msub>
<mml:mo>=</mml:mo>
<mml:mn>0.60</mml:mn>
<mml:mo>±</mml:mo>
<mml:mn>0.06</mml:mn>
</mml:mrow>
</mml:math></jats:alternatives></jats:inline-formula> (when the Universe change from an decelerated phase to an accelerated one). These results are in contrast with previous work that favors CC scenario, nevertheless our lensing analysis is in agreement with a formerly reported conclusion suggesting that the variable brane tension model is able to source a late cosmic acceleration without an extra fluid as in the standard one.</jats:p>