Ladder symmetry: The necessary and sufficient condition for vanishing Love numbers

Explicit construction of the energy-momentum tensor in the large <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mi>N</mml:mi> </mml:math> limit

Plasma flow in force-free magnetospheres: Two-fluid model near pulsars and black holes

Adiabatic initial conditions for a particle gas in cosmology

Scalar leptoquark contributions to the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mi>g</mml:mi> <mml:mi>g</mml:mi> <mml:mo>→</mml:mo> <mml:mi>Z</mml:mi> <mml:mi>h</mml:mi> </mml:mrow> </mml:math> process

Effective field theory of coupled dark energy and dark matter

Ladder symmetry: The necessary and sufficient condition for vanishing Love numbers

Explicit construction of the energy-momentum tensor in the large <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mi>N</mml:mi> </mml:math> limit

Plasma flow in force-free magnetospheres: Two-fluid model near pulsars and black holes

Adiabatic initial conditions for a particle gas in cosmology

Scalar leptoquark contributions to the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mi>g</mml:mi> <mml:mi>g</mml:mi> <mml:mo>→</mml:mo> <mml:mi>Z</mml:mi> <mml:mi>h</mml:mi> </mml:mrow> </mml:math> process

Effective field theory of coupled dark energy and dark matter