Search results for "BD"

showing 10 items of 3363 documents

N order solutions with multi-parameters to the Boussinesq and KP equations and the degenerate rational case

2021

From elementary exponential functions which depend on several parameters, we construct multi-parametric solutions to the Boussinesq equation. When we perform a passage to the limit when one of these parameters goes to 0, we get rational solutions as a quotient of a polynomial of degree N (N + 1) − 2 in x and t, by a polynomial of degree N (N + 1) in x and t for each positive integer N depending on 3N parameters. We restrict ourself to give the explicit expressions of these rational solutions for N = 1 until N = 3 to shortened the paper. We easily deduce the corresponding explicit rational solutions to the Kadomtsev Petviashvili equation for the same orders from 1 to 3.

47.35.Fg47.10A-rational solutions PACS numbers : 33Q55[MATH.MATH-MP]Mathematics [math]/Mathematical Physics [math-ph]47.54.Bd37K10[MATH.MATH-MP] Mathematics [math]/Mathematical Physics [math-ph]Boussinesq equationKadomtsev Petviashvili equation
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From particular polynomials to rational solutions to the PII equation

2022

The Painlevé equations were derived by Painlevé and Gambier in the years 1895 − 1910. Given a rational function R in w, w ′ and analytic in z, they searched what were the second order ordinary differential equations of the form w ′′ = R(z, w, w ′) with the properties that the singularities other than poles of any solution or this equation depend on the equation only and not of the constants of integration. They proved that there are fifty equations of this type, and the Painlevé II is one of these. Here, we construct solutions to the Painlevé II equation (PII) from particular polynomials. We obtain rational solutions written as a derivative with respect to the variable x of a logarithm of a…

47.35.Fg47.54.Bd Painlevé equation II rational solutions determinantsnumbers : 33Q5547.10A-rational solutions47.54.Bd Painlevé equation IIdeterminants37K10[MATH.MATH-MP] Mathematics [math]/Mathematical Physics [math-ph]
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Multi-parameters rational solutions to the mKdV equation

2021

N-order solutions to the modified Korteweg-de Vries (mKdV) equation are given in terms of a quotient of two wronskians of order N depending on 2N real parameters. When one of these parameters goes to 0, we succeed to get for each positive integer N , rational solutions as a quotient of polynomials in x and t depending on 2N real parameters. We construct explicit expressions of these rational solutions for orders N = 1 until N = 6.

47.35.FgNonlinear Sciences::Exactly Solvable and Integrable Systemswronskians47.10A-rational solutions PACS numbers : 33Q55[MATH.MATH-MP]Mathematics [math]/Mathematical Physics [math-ph]47.54.Bd[MATH.MATH-MP] Mathematics [math]/Mathematical Physics [math-ph]37K10mKdV equation
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Other patterns for the first and second order rational solutions to the KPI equation

2022

We present rational solutions to the Kadomtsev-Petviashvili equation (KPI) in terms of polynomials in x, y and t depending on several real parameters. We get an infinite hierarchy of rational solutions written as a quotient of a polynomial of degree 2N (N + 1) − 2 in x, y and t by a polynomial of degree 2N (N + 1) in x, y and t, depending on 2N − 2 real parameters for each positive integer N. We construct explicit expressions of the solutions in the simplest cases N = 1 and N = 2 and we study the patterns of their modulus in the (x, y) plane for different values of time t and parameters. In particular, in the study of these solutions, we see the appearance not yet observed of three pairs of…

47.35.Fgnumbers : 33Q5547.10A-47.54.Bd37K10[MATH.MATH-MP] Mathematics [math]/Mathematical Physics [math-ph]
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From particular polynomials to rational solutions to the KPI equation

2022

We construct solutions to the Kadomtsev-Petviashvili equation (KPI) from particular polynomials. We obtain rational solutions written as a second derivative with respect to the variable x of a logarithm of a determinant of order n. So we get with this method an infinite hierarchy of rational solutions to the KPI equation. We give explicitly the expressions of these solutions for the first five orders.

47.35.Fgnumbers : 33Q5547.10A-47.54.Bd37K10[MATH.MATH-MP] Mathematics [math]/Mathematical Physics [math-ph]
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Rational solutions of order N to the KPI equation with multi-parameters and the explicit case of order 3

2022

We present multiparametric rational solutions to the Kadomtsev-Petviashvili equation (KPI). These solutions of order N depend on 2N − 2 real parameters. Explicit expressions of the solutions at order 3 are given. They can be expressed as a quotient of a polynomial of degree 2N (N + 1) − 2 in x, y and t by a polynomial of degree 2N (N + 1) in x, y and t, depending on 2N − 2 real parameters. We study the patterns of their modulus in the (x,y) plane for different values of time t and parameters.

47.35.Fgnumbers : 33Q5547.10A-47.54.Bd37K10[MATH.MATH-MP] Mathematics [math]/Mathematical Physics [math-ph]
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Solutions to the Gardner equation with multiparameters and the rational case

2022

We construct solutions to the Gardner equation in terms of trigonometric and hyperbolic functions, depending on several real parameters. Using a passage to the limit when one of these parameters goes to 0, we get, for each positive integer N , rational solutions as a quotient of polynomials in x and t depending on 2N parameters. We construct explicit expressions of these rational solutions for orders N = 1 until N = 3. We easily deduce solutions to the mKdV equation in terms of wronskians as well as rational solutions depending on 2N real parameters.

47.35.Fgwronskians47.10A-rational solutions PACS numbers : 33Q5547.54.BdGardner equation37K10[MATH.MATH-MP] Mathematics [math]/Mathematical Physics [math-ph]
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Wind accretion in the massive X-ray binary 4U 2206+54: abnormally slow wind and a moderately eccentric orbit

2006

Massive X-ray binaries are usually classified depending on the properties of the donor star in classical, supergiant and Be X-ray binaries. The massive X-ray binary 4U 2206+54 does not fit in any of these groups, and deserves a detailed study to understand how the transfer of matter and the accretion on to the compact object take place. To this end we study an IUE spectrum of the donor and obtain a wind terminal velocity (v_inf) of ~350 km/s, which is abnormally slow for its spectral type. We also analyse here more than 9 years of available RXTE/ASM data. We study the long-term X-ray variability of the source and find it to be similar to that observed in the wind-fed supergiant system Vela …

4U 2206+54X-ray binaryBinary numberFOS: Physical sciencesOutflows Emission-lineOrbital eccentricityAstrophysicsWindsCompact starUNESCO::ASTRONOMÍA Y ASTROFÍSICAVelaAstrophysicsIndividual starsPhysicsAstrophysics (astro-ph)BD +53◦2790BeAstronomy and AstrophysicsOrbital period:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Accretion (astrophysics)X-rays binariesX-rays individualsX-rays binaries ; X-rays individuals ; 4U 2206+54 ; Individual stars ; BD +53◦2790 ; Winds ; Outflows Emission-line ; BeSpace and Planetary ScienceUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaSupergiant:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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"P_AntiLambda vs. pT (5.02TeV, 5-15%)" of "Global polarization of $\Lambda$ and $\overline{\Lambda}$ hyperons in Pb-Pb collisions at the LHC"

2021

The $\bar\Lambda$ global polarization as function of transverse momentum ($p_{\mathrm{T}}$) for 5-15% centrality in Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=5.02$~TeV.

5020.0High Energy Physics::PhenomenologyPb Pb --> LAMBDA XP_LAMBDAHigh Energy Physics::ExperimentNuclear Experiment$\Lambda$ global polarization
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"P_AntiLambda vs. wide centrality bins (5.02 TeV)" of "Global polarization of $\Lambda$ and $\overline{\Lambda}$ hyperons in Pb-Pb collisions at the …

2021

The $\bar\Lambda$ global polarization as function of centrality for Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=5.02$~TeV.

5020.0P_ANTI-LAMBDAHigh Energy Physics::PhenomenologyPb Pb --> ANTI-LAMBDA XHigh Energy Physics::ExperimentNuclear Experiment$\bar\Lambda$ global polarization
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