☆ 4.8 Article

Gravitational Waves from Compact Dark Objects in Neutron Stars

PHYSICAL REVIEW LETTERS (2019)

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PHYSICAL REVIEW LETTERS

卷 122, 期 7, 页码 -

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AMER PHYSICAL SOC

DOI: 10.1103/PhysRevLett.122.071102

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Physics, Multidisciplinary

资金

DOE [DE-FG02-87ER40365, DE-SC0018083]
National Science Foundation [PHY-1430152]
U.S. Department of Energy [DE-FG02-00ER41132]

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摘要

Dark matter could be composed of compact dark objects (CDOs). We find that the oscillation of CDOs inside neutron stars can be a detectable source of gravitational waves (GWs). The GW strain amplitude depends on the mass of the CDO, and its frequency is typically in the range 3-5 kHz as determined by the central density of the star. In the best cases, LIGO may be sensitive to CDO masses greater than or of order 10(-8) M-circle dot.

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Lee, J. Lee, K. Lee, R. Lee, J. Lehmann, A. Lemaitre, E. Leon, M. Leonardi, N. Leroy, N. Letendre, Y. Levin, J. N. Leviton, A. K. Y. Li, B. Li, J. Li, K. L. Li, T. G. F. Li, X. Li, C. -Y. Lin, F. -K. Lin, F. -L. Lin, H. L. Lin, L. C. -C. Lin, F. Linde, S. D. Linker, J. N. Linley, T. B. Littenberg, G. C. Liu, J. Liu, K. Liu, X. Liu, M. Llorens-Monteagudo, R. K. L. Lo, A. Lockwood, M. L. Lollie, L. T. London, A. Longo, D. Lopez, M. Lorenzini, V. Loriette, M. Lormand, G. Losurdo, J. D. Lough, C. O. Lousto, G. Lovelace, H. Luck, D. Lumaca, A. P. Lundgren, L. -W. Luo, R. Macas, M. MacInnis, D. M. Macleod, I. A. O. MacMillan, A. Macquet, I. Magana Hernandez, F. Magana-Sandoval, C. Magazzu, R. M. Magee, R. Maggiore, E. Majorana, I. Maksimovic, S. Maliakal, A. Malik, N. Man, V. Mandic, V. Mangano, J. L. Mango, G. L. Mansell, M. Manske, M. Mantovani, M. Mapelli, F. Marchesoni, M. Marchio, F. Marion, Z. Mark, S. Marka, Z. Marka, C. Markakis, A. S. Markosyan, A. Markowitz, E. Maros, A. Marquina, S. Marsat, F. Martelli, I. W. Martin, R. M. Martin, M. Martinez, V. Martinez, K. Martinovic, D. V. Martynov, E. J. Marx, H. Masalehdan, K. Mason, E. Massera, A. Masserot, T. J. Massinger, M. Masso-Reid, S. Mastrogiovanni, A. Matas, M. Mateu-Lucena, F. Matichard, M. Matiushechkina, N. Mavalvala, J. J. McCann, R. McCarthy, D. E. McClelland, P. McClincy, S. McCormick, L. McCuller, G. I. McGhee, S. C. McGuire, C. McIsaac, J. McIver, D. J. McManus, T. Mcrae, S. T. McWilliams, D. Meacher, M. Mehmet, A. K. Mehta, A. Melatos, D. A. Melchor, G. Mendell, A. Menendez-Vazquez, C. S. Menoni, R. A. Mercer, L. Mereni, K. Merfeld, E. L. Merilh, J. D. Merritt, M. Merzougui, S. Meshkov, C. Messenger, C. Messick, P. M. Meyers, F. Meylahn, A. Mhaske, A. Miani, H. Miao, I. Michaloliakos, C. Michel, Y. Michimura, H. Middleton, L. Milano, A. L. Miller, M. Millhouse, J. C. Mills, E. Milotti, M. C. Milovich-Goff, O. Minazzoli, Y. Minenkov, N. Mio, Ll. M. Mir, A. Mishkin, C. Mishra, T. Mishra, T. Mistry, S. Mitra, V. P. Mitrofanov, G. Mitselmakher, R. Mittleman, O. Miyakawa, A. Miyamoto, Y. Miyazaki, K. Miyo, S. Miyoki, Geoffrey Mo, K. Mogushi, S. R. P. Mohapatra, S. R. Mohite, I. Molina, M. Molina-Ruiz, M. Mondin, M. Montani, C. J. Moore, D. Moraru, F. Morawski, A. More, C. Moreno, G. Moreno, Y. Mori, S. Morisaki, Y. Moriwaki, B. Mours, C. M. Mow-Lowry, S. Mozzon, F. Muciaccia, Arunava Mukherjee, D. Mukherjee, Soma Mukherjee, Subroto Mukherjee, N. Mukund, A. Mullavey, J. Munch, E. A. Muniz, P. G. Murray, R. Musenich, S. L. Nadji, K. Nagano, S. Nagano, A. Nagar, K. Nakamura, H. Nakano, M. Nakano, R. Nakashima, Y. Nakayama, I. Nardecchia, T. Narikawa, L. Naticchioni, B. Nayak, R. K. Nayak, R. Negishi, B. F. Neil, J. Neilson, G. Nelemans, T. J. N. Nelson, M. Nery, A. Neunzert, K. Y. Ng, S. W. S. Ng, C. Nguyen, P. Nguyen, T. Nguyen, L. Nguyen Quynh, W. -T. Ni, S. A. Nichols, A. Nishizawa, S. Nissanke, F. Nocera, M. Noh, M. Norman, C. North, S. Nozaki, L. K. Nuttall, J. Oberling, B. D. O'Brien, Y. Obuchi, J. O'Dell, W. Ogaki, G. Oganesyan, J. J. Oh, K. Oh, S. H. Oh, M. Ohashi, N. Ohishi, M. Ohkawa, F. Ohme, H. Ohta, M. A. Okada, Y. Okutani, K. Okutomi, C. Olivetto, K. Oohara, C. Ooi, R. Oram, B. O'Reilly, R. G. Ormiston, N. D. Ormsby, L. F. Ortega, R. O'Shaughnessy, E. O'Shea, S. Oshino, S. Ossokine, C. Osthelder, S. Otabe, D. J. Ottaway, H. Overmier, A. E. Pace, G. Pagano, M. A. Page, G. Pagliaroli, A. Pai, S. A. Pai, J. R. Palamos, O. Palashov, C. Palomba, K. Pan, P. K. Panda, H. Pang, P. T. H. Pang, C. Pankow, F. Pannarale, B. C. Pant, F. Paoletti, A. Paoli, A. Paolone, A. Parisi, J. Park, W. Parker, D. Pascucci, A. Pasqualetti, R. Passaquieti, D. Passuello, M. Patel, B. Patricelli, E. Payne, T. C. Pechsiri, M. Pedraza, M. Pegoraro, A. Pele, F. E. Pena Arellano, S. Penn, A. Perego, A. Pereira, T. Pereira, C. J. Perez, C. Perigois, A. Perreca, S. Perries, J. Petermann, D. Petterson, H. P. Pfeiffer, K. A. Pham, K. S. Phukon, O. J. Piccinni, M. Pichot, M. Piendibene, F. Piergiovanni, L. Pierini, V. Pierro, G. Pillant, F. Pilo, L. Pinard, I. M. Pinto, B. J. Piotrzkowski, K. Piotrzkowski, M. Pirello, M. Pitkin, E. Placidi, W. Plastino, C. Pluchar, R. Poggiani, E. Polini, D. Y. T. Pong, S. Ponrathnam, P. Popolizio, E. K. Porter, J. Powell, M. Pracchia, T. Pradier, A. K. Prajapati, K. Prasai, R. Prasanna, G. Pratten, T. Prestegard, M. Principe, G. A. Prodi, L. Prokhorov, P. Prosposito, L. Prudenzi, A. Puecher, M. Punturo, F. Puosi, P. Puppo, M. Purrer, H. Qi, V. Quetschke, J. Quinonez, R. Quitzow-James, F. J. Raab, G. Raaijmakers, H. Radkins, N. Radulesco, P. Raffai, S. X. Rail, S. Raja, C. Rajan, K. E. Ramirez, T. D. Ramirez, A. Ramos-Buades, J. Rana, P. Rapagnani, U. D. Rapol, B. Ratto, V. Raymond, N. Raza, M. Razzano, J. Read, L. A. Rees, T. Regimbau, L. Rei, S. Reid, D. H. Reitze, P. Relton, P. Rettegno, F. Ricci, C. J. Richardson, J. W. Richardson, L. Richardson, P. M. Ricker, G. Riemenschneider, K. Riles, M. Rizzo, N. A. Robertson, R. Robie, F. Robinet, A. Rocchi, J. A. Rocha, S. Rodriguez, R. D. Rodriguez-Soto, L. Rolland, J. G. Rollins, V. J. Roma, M. Romanelli, R. Romano, C. L. Romel, A. Romero, I. M. Romero-Shaw, J. H. Romie, C. A. Rose, D. Rosinska, S. G. Rosofsky, M. P. Ross, S. Rowan, S. J. Rowlinson, Santosh Roy, Soumen Roy, D. Rozza, P. Ruggi, K. Ryan, S. Sachdev, T. Sadecki, J. Sadiq, N. Sago, S. Saito, Y. Saito, K. Sakai, Y. Sakai, M. Sakellariadou, Y. Sakuno, O. S. Salafia, L. Salconi, M. Saleem, F. Salemi, A. Samajdar, E. J. Sanchez, J. H. Sanchez, L. E. Sanchez, N. Sanchis-Gual, J. R. Sanders, A. Sanuy, T. R. Saravanan, N. Sarin, B. Sassolas, H. Satari, S. Sato, T. Sato, O. Sauter, R. L. Savage, V. Savant, T. Sawada, D. Sawant, H. L. Sawant, S. Sayah, D. Schaetzl, M. Scheel, J. Scheuer, A. Schindler-Tyka, P. Schmidt, R. Schnabel, M. Schneewind, R. M. S. Schofield, A. Schonbeck, B. W. Schulte, B. F. Schutz, E. Schwartz, J. Scott, S. M. Scott, M. Seglar-Arroyo, E. Seidel, T. Sekiguchi, Y. Sekiguchi, D. Sellers, A. Sergeev, A. S. Sengupta, N. Sennett, D. Sentenac, E. G. Seo, V. Sequino, Y. Setyawati, T. Shaffer, M. S. Shahriar, B. Shams, L. Shao, S. Sharifi, A. Sharma, P. Sharma, P. Shawhan, N. S. Shcheblanov, H. Shen, S. Shibagaki, M. Shikauchi, R. Shimizu, T. Shimoda, K. Shimode, R. Shink, H. Shinkai, T. Shishido, A. Shoda, D. H. Shoemaker, D. M. Shoemaker, K. Shukla, S. ShyamSundar, M. Sieniawska, D. Sigg, L. P. Singer, D. Singh, N. Singh, A. Singha, A. M. Sintes, V. Sipala, V. Skliris, B. J. J. Slagmolen, T. J. Slaven-Blair, J. Smetana, J. R. Smith, R. J. E. Smith, S. N. Somala, K. Somiya, E. J. Son, K. Soni, S. Soni, B. Sorazu, V. Sordini, F. Sorrentino, N. Sorrentino, H. Sotani, R. Soulard, T. Souradeep, E. Sowell, V. Spagnuolo, A. P. Spencer, M. Spera, A. K. Srivastava, V. Srivastava, K. Staats, C. Stachie, D. A. Steer, J. Steinlechner, S. Steinlechner, D. J. Stops, M. Stover, K. A. Strain, L. C. Strang, G. Stratta, A. Strunk, R. Sturani, A. L. Stuver, J. Sudbeck, S. Sudhagar, V. Sudhir, R. Sugimoto, H. G. Suh, T. Z. Summerscales, H. Sun, L. Sun, S. Sunil, A. Sur, J. Suresh, P. J. Sutton, Takamasa Suzuki, Toshikazu Suzuki, B. L. Swinkels, M. J. Szczepanczyk, P. Szewczyk, M. Tacca, H. Tagoshi, S. C. Tait, H. Takahashi, R. Takahashi, A. Takamori, S. Takano, H. Takeda, M. Takeda, C. Talbot, H. Tanaka, Kazuyuki Tanaka, Kenta Tanaka, Taiki Tanaka, Takahiro Tanaka, A. J. Tanasijczuk, S. Tanioka, D. B. Tanner, D. Tao, A. Tapia, E. N. Tapia San Martin, E. N. Tapia San Martin, J. D. Tasson, S. Telada, R. Tenorio, L. Terkowski, M. Test, M. P. Thirugnanasambandam, M. Thomas, P. Thomas, J. E. Thompson, S. R. Thondapu, K. A. Thorne, E. Thrane, Shubhanshu Tiwari, Srishti Tiwari, V. Tiwari, K. Toland, A. E. Tolley, T. Tomaru, Y. Tomigami, T. Tomura, M. Tonelli, A. Torres-Forne, C. I. Torrie, I. Tosta e Melo, D. Toyra, A. Trapananti, F. Travasso, G. Traylor, M. C. Tringali, A. Tripathee, L. Troiano, A. Trovato, L. Trozzo, R. J. Trudeau, D. S. Tsai, D. Tsai, K. W. Tsang, T. Tsang, J-S. Tsao, M. Tse, R. Tso, K. Tsubono, S. Tsuchida, L. Tsukada, D. Tsuna, T. Tsutsui, T. Tsuzuki, M. Turconi, D. Tuyenbayev, A. S. Ubhi, N. Uchikata, T. Uchiyama, R. P. Udall, A. Ueda, T. Uehara, K. Ueno, G. Ueshima, D. Ugolini, C. S. Unnikrishnan, F. Uraguchi, A. L. Urban, T. Ushiba, S. A. Usman, A. C. Utina, H. Vahlbruch, G. Vajente, A. Vajpeyi, G. Valdes, M. Valentini, V. Valsan, N. van Bakel, M. van Beuzekom, J. F. J. van den Brand, C. Van den Broeck, D. C. Vander-Hyde, L. van der Schaaf, J. V. van Heijningen, M. H. P. M. van Putten, M. Vardaro, A. F. Vargas, V. Varma, M. Vasuth, A. Vecchio, G. Vedovato, J. Veitch, P. J. Veitch, K. Venkateswara, J. Venneberg, G. Venugopalan, D. Verkindt, Y. Verma, D. Veske, F. Vetrano, A. Vicere, A. D. Viets, V. Villa-Ortega, J. -Y. Vinet, S. Vitale, T. Vo, H. Vocca, E. R. G. von Reis, J. von Wrangel, C. Vorvick, S. P. Vyatchanin, L. E. Wade, M. Wade, K. J. Wagner, R. C. Walet, M. Walker, G. S. Wallace, L. Wallace, S. Walsh, J. Wang, J. Z. Wang, W. H. Wang, R. L. Ward, J. Warner, M. Was, T. Washimi, N. Y. Washington, J. Watchi, B. Weaver, L. Wei, M. Weinert, A. J. Weinstein, R. Weiss, C. M. Weller, F. Wellmann, L. Wen, P. Wessels, J. W. Westhouse, K. Wette, J. T. Whelan, D. D. White, B. F. Whiting, C. Whittle, D. Wilken, D. Williams, M. J. Williams, A. R. Williamson, J. L. Willis, B. Willke, D. J. Wilson, W. Winkler, C. C. Wipf, T. Wlodarczyk, G. Woan, J. Woehler, J. K. Wofford, I. C. F. Wong, C. Wu, D. S. Wu, H. Wu, S. Wu, D. M. Wysocki, L. Xiao, W-R. Xu, T. Yamada, H. Yamamoto, Kazuhiro Yamamoto, Kohei Yamamoto, T. Yamamoto, K. Yamashita, R. Yamazaki, F. W. Yang, L. Yang, Yang, Yi Yang, Z. Yang, M. J. Yap, D. W. Yeeles, A. B. Yelikar, M. Ying, K. Yokogawa, J. Yokoyama, T. Yokozawa, A. Yoon, T. Yoshioka, Hang Yu, Haocun Yu, H. Yuzurihara, A. Zadrozny, M. Zanolin, S. Zeidler, T. Zelenova, J. -P. Zendri, M. Zevin, M. Zhan, H. Zhang, J. Zhang, L. Zhang, R. Zhang, T. Zhang, C. Zhao, G. Zhao, Yue Zhao, Yuhang Zhao, Z. Zhou, X. J. Zhu, Z. -H. Zhu, A. Zicoschi, M. E. Zucker, J. Zweizig, D. Antonopoulou, Z. Arzoumanian, T. Enoto, C. M. Espinoza, S. Guillot

Summary: Analysis of data from PSR J0537-6910 in the LIGO-Virgo Collaboration observing run O3 was conducted to search for continuous gravitational-wave emission due to r-modes, although no expected signals were detected. The study reported upper limits on the amplitude of gravitational waves, improving on previous limits and placing stringent constraints on theoretical models for the spin-down in the pulsar.

ASTROPHYSICAL JOURNAL (2021)

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Article Astronomy & Astrophysics

Dynamical tides in superfluid neutron stars

A. Passamonti, N. Andersson, P. Pnigouras

Summary: This study focuses on the tidal response of a superfluid neutron star in a binary system and finds that superfluid physics has a negligible impact on static tidal deformation. The overwhelming contribution to the Love number is from the ordinary fundamental mode. Strong entrainment has a significant impact on superfluid modes, but the results for the dynamical tide are similar to the static limit.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2022)

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Article Astronomy & Astrophysics

Modelling neutron star mountains in relativity

Fabian Gittins, Nils Andersson

Summary: This paper discusses the upper limits on quadrupole deformations of rapidly spinning, deformed neutron stars and the size of mountains before the neutron star crust fractures. By considering a range of models obtained from chiral effective field theory, it is found that the derived mountains depend on the equation of state.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

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Article Astronomy & Astrophysics

Ultra-compact X-ray binaries as dual-line gravitational-wave sources

A. G. Suvorov

Summary: Ultra-compact X-ray binaries are promising sources for both space-borne and ground-based gravitational-wave interferometers. Two Galactic systems have been identified as potentially detectable by both LISA and aLIGO simultaneously, providing percent-level constraints on neutron star properties.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

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Article Physics, Multidisciplinary

Actinide Crystallization and Fission Reactions in Cooling White Dwarf Stars

C. J. Horowitz, M. E. Caplan

Summary: Research suggests that as a white dwarf starts to crystallize, the first solids formed may be highly enriched in actinides, potentially leading to a fission chain reaction and ignition of carbon burning, resulting in a thermonuclear supernova explosion. This mechanism could offer an explanation for supernovae with sub-Chandrasekhar ejecta masses and short delay times.

PHYSICAL REVIEW LETTERS (2021)

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Article Physics, Multidisciplinary

Implications of PREX-2 on the Equation of State of Neutron-Rich Matter

Brendan T. Reed, F. J. Fattoyev, C. J. Horowitz, J. Piekarewicz

Summary: Laboratory experiments sensitive to the equation of state of neutron rich matter in the vicinity of nuclear saturation density provide crucial data connecting terrestrial experiments to astronomical observations. The neutron skin thickness of Pb-208 further constrains the density dependence of the symmetry energy. The impact of a stiff symmetry energy on critical neutron-star observables is studied.

PHYSICAL REVIEW LETTERS (2021)

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Article Astronomy & Astrophysics

Modeling the Galactic Neutron Star Population for Use in Continuous Gravitational-wave Searches

Brendan T. Reed, Alex Deibel, C. J. Horowitz

Summary: Searches for continuous gravitational waves from unknown Galactic neutron stars provide limits on the shapes of neutron stars. Using a simple model of the spatial and spin distribution of Galactic neutron stars, the total number of neutron stars probed can be estimated, aiding in optimizing future searches with improved sensitivity. Third-generation GW detectors may greatly increase the number of neutron stars probed to a given ellipticity.

ASTROPHYSICAL JOURNAL (2021)

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Article Physics, Multidisciplinary

New Measurements of the Beam-Normal Single Spin Asymmetry in Elastic Electron Scattering over a Range of Spin-0 Nuclei

D. Adhikari, H. Albataineh, D. Androic, K. Aniol, D. S. Armstrong, T. Averett, C. Ayerbe Gayoso, S. Barcus, V. Bellini, R. S. Beminiwattha, J. F. Benesch, H. Bhatt, D. Bhatta Pathak, D. Bhetuwal, B. Blaikie, J. Boyd, Q. Campagna, A. Camsonne, G. D. Cates, Y. Chen, C. Clarke, J. C. Cornejo, S. Covrig Dusa, M. M. Dalton, P. Datta, A. Deshpande, D. Dutta, C. Feldman, E. Fuchey, C. Gal, D. Gaskell, T. Gautam, M. Gericke, C. Ghosh, I. Halilovic, J. -O. Hansen, F. Hauenstein, W. Henry, C. J. Horowitz, C. Jantzi, S. Jian, S. Johnston, D. C. Jones, B. Karki, S. Kakkar, S. Katugampola, C. E. Keppel, P. M. King, D. E. King, M. Knauss, K. S. Kumar, T. Kutz, N. Lashley-Colthirst, G. Leverick, H. Liu, N. Liyange, S. Malace, J. Mammei, R. Mammei, M. McCaughan, D. McNulty, D. Meekins, C. Metts, R. Michaels, M. Mihovilovic, M. M. Mondal, J. Napolitano, D. Nikolaev, M. N. H. Rashad, V. Owen, C. Palatchi, J. Pan, B. Pandey, S. Park, K. D. Paschke, M. Petrusky, M. L. Pitt, S. Premathilake, A. J. R. Puckett, B. Quinn, R. Radloff, S. Rahman, A. Rathnayake, B. T. Reed, P. E. Reimer, R. Richards, S. Riordan, Y. Roblin, S. Seeds, A. Shahinyan, P. A. Souder, L. Tang, M. Thiel, Y. Tian, G. M. Urciuoli, E. W. Wertz, B. Wojtsekhowski, W. Xiong, B. Yale, T. Ye, A. Zec, W. Zhang, J. Zhang, X. Zheng

Summary: Precision determinations of the beam-normal single spin asymmetries (A(n)) in the elastic scattering of 0.95 and 2.18 GeV electrons off C-12, Ca-40, Ca-48, and Pb-208 were reported. The measurement results for Ca-40 and Ca-48 are similar to that of C-12, consistent with expectations and validating the theoretical calculations for nuclei with Z ≤ 20. However, the A(n) measurements for Pb-208 show significant disagreement with the results for Z ≤ 20 nuclei, indicating the need for further investigation.

PHYSICAL REVIEW LETTERS (2022)

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Article Astronomy & Astrophysics

Ignition of Carbon Burning from Nuclear Fission in Compact Stars

C. J. Horowitz

Summary: A new mechanism involving nuclear fission chain reactions in a white dwarf has been proposed, which could lead to thermonuclear ignition and the production of a Type Ia supernova or other astrophysical transients.

ASTROPHYSICAL JOURNAL LETTERS (2022)

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Article Astronomy & Astrophysics

Neutron star crust can support a large ellipticity

J. A. Morales, C. J. Horowitz

Summary: Non-axisymmetrical deformations of the crust on rapidly rotating neutron stars can generate continuous gravitational waves, with a maximum ellipticity of 7.4 x 10(-6).

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2022)

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Article Astronomy & Astrophysics

Detectability of subsolar mass neutron stars through a template bank search

Ananya Bandopadhyay, Brendan Reed, Surendra Padamata, Erick Leon, C. J. Horowitz, Duncan A. Brown, David Radice, F. J. Fattoyev, J. Piekarewicz

Summary: We investigate the detectability of gravitational-wave signals from subsolar-mass binary neutron star systems using current ground-based detectors. Finite size effects and lower merger frequencies of neutron stars significantly impact the sensitivity of these detectors. By simulating a matched-filter search with injected signals, we calculate the reduction in sensitivity and obtain an upper limit on the merger rate. The discovery of low-mass neutron stars would provide new insights into their formation mechanisms and constrain dense nuclear matter.

PHYSICAL REVIEW D (2023)

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Article Physics, Nuclear

Nuclear fission reaction simulations in compact stars

Alex Deibel, M. E. Caplan, C. J. Horowitz

Summary: Scientists simulated the reaction network of actinide-rich solids in a cooling white dwarf and found that under moderate uranium enrichment, neutron capture can breed additional fissile nuclei, leading to the fission of a significant fraction of U and Th nuclei during the chain reaction.

PHYSICAL REVIEW C (2022)

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Article Astronomy & Astrophysics

Cooling Delays from Iron Sedimentation and Iron Inner Cores in White Dwarfs

M. E. Caplan, I. F. Freeman, C. J. Horowitz, A. Cumming, E. P. Bellinger

Summary: This study suggests that white dwarfs may have inner cores made of iron which separate into mesoscopic crystallites. The associated cooling delays could be up to a Gyr for low-mass white dwarfs but are only around 0.1 Gyr for massive white dwarfs. The heating from this mechanism is insufficient to fully explain certain phenomena.

ASTROPHYSICAL JOURNAL LETTERS (2021)

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Article Astronomy & Astrophysics

Total energy in supernova neutrinos and the tidal deformability and binding energy of neutron stars

Brendan Reed, C. J. Horowitz

PHYSICAL REVIEW D (2020)

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Article Physics, Nuclear

GW190814: Impact of a 2.6 solar mass neutron star on the nucleonic equations of state

F. J. Fattoyev, C. J. Horowitz, J. Piekarewicz, Brendan Reed

PHYSICAL REVIEW C (2020)

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Article Physics, Nuclear

Measuring the surface thickness of the weak charge density of nuclei

Brendan T. Reed, Z. Jaffe, C. J. Horowitz, C. Sfienti

PHYSICAL REVIEW C (2020)

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Article Astronomy & Astrophysics

Nuclear and dark matter heating in massive white dwarf stars

C. J. Horowitz

PHYSICAL REVIEW D (2020)

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Article Physics, Nuclear

Insights into nuclear saturation density from parity-violating electron scattering

C. J. Horowitz, J. Piekarewicz, Brendan Reed

PHYSICAL REVIEW C (2020)

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Article Physics, Nuclear

Fast neutrino cooling of nuclear pasta in neutron stars: Molecular dynamics simulations

Zidu Lin, Matthew E. Caplan, Charles J. Horowitz, Cecilia Lunardini

PHYSICAL REVIEW C (2020)

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