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Иш: Identifying unstable regions in collapsing stars using radial perturbation techniques and relativistic corrections
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
S. Perlmutter, G. Aldering, G. Goldhaber +30
Мақола1999103 иқтибосABI<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mi>T</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>gravity
Tiberiu Harko, Francisco S. N. Lobo, Shin’ichi Nojiri +1
Мақола201165 иқтибосABIUnified cosmic history in modified gravity: From <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si10.gif" display="inline" overflow="scroll"><mml:mi>F</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math> theory to Lorentz non-invariant models
Shin’ichi Nojiri, Sergei D. Odintsov
Мақола201139 иқтибосABIDynamical stability of new wormhole solutions via cold dark matter and solitonic quantum wave halos in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.svg" display="inline" id="d1e3341"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant="script">R</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mrow><mml:mi mathvariant="script">L</mml:mi></mml:mrow><mml:mrow><mml:mi>m</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> gravity
G. Mustafa, Faisal Javed, S. K. Maurya +2
Мақола202411 иқтибосABICosmological and solar system consequences of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mi>T</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow></mml:math>gravity models
Hamid Shabani, Mehrdad Farhoudi
Мақола20148 иқтибосABICylindrical wormholes and electromagnetic field
M. Yousaf, M. Z. Bhatti, Z. Yousaf
Мақола20238 иқтибосABI